897:
856:. Indeed, the spectrographic presence of these elements, along with a notable absence of hydrogen, were one of the original diagnostic criteria for classifying a star as WolfâRayet. It is these enriched layers of the photosphere that are lost in repeating pulses. Once distant from the surface, the carbon fraction of this ejected material begins to glow at approximately 1000
1024:. This helium burning provided a burst of radiation pressure that propagated through the star, up to its surface. The star began to inflate, though this increase in size was only temporary. The thin shell of helium fusion eventually caused enough expansion to moderate, or even extinguish its own reaction. The star once again began to collapse.
28:
985:
some variety of spiral. This is thought to be the result of the dueling solar winds in binary systems, which compress clouds of dust into distinct shock fronts. The concentric nature of WR 140's dust shells is not well understood, although it may be related to nuclear processes in the WolfâRayet star's core.
1268:
Cutri, Roc M.; Skrutskie, Michael F.; Van Dyk, Schuyler D.; Beichman, Charles A.; Carpenter, John M.; Chester, Thomas; Cambresy, Laurent; Evans, Tracey E.; Fowler, John W.; Gizis, John E.; Howard, Elizabeth V.; Huchra, John P.; Jarrett, Thomas H.; Kopan, Eugene L.; Kirkpatrick, J. Davy; Light, Robert
1031:
into space. Following this, the star began to fuse helium at a greater rate and temporarily regained its former radiation pressure. This helium fusion once again stalled, and the subsequent gravitational collapse dislodged another layer of photosphere into space. These pulses will continue as long as
984:
collide with the dust formation created by the WolfâRayet star, causing the unusual bulges and angles in the concentric shells of dust. The dust typically emitted by WolfâRayet systems is not so coherent or concentric as those of WR 140. The dust lanes around WolfâRayets are most commonly observed as
1751:
Fahed, R.; Moffat, A. F. J.; Zorec, J.; Eversberg, T.; Chené, A. N.; Alves, F.; Arnold, W.; Bergmann, T.; Corcoran, M. F.; Correia Viegas, N. G.; Dougherty, S. M.; Fernando, A.; Frémat, Y.; Gouveia
Carreira, L. F.; Hunger, T.; Knapen, J. H.; Leadbeater, R.; Marques Dias, F.; Martayan, C.; Morel, T.;
1042:
The immense surface temperature of WolfâRayet stars (up to 210,000 K) produces intense ultraviolet radiation, enough to make 20 or more layers visible to instrumentation. The distance between the concentric shells of ejected material corresponds to the time between one faltering of the star's
1532:
Monnier, J. D.; Zhao, Ming; Pedretti, E.; Millan-Gabet, R.; Berger, J.-P.; Traub, W.; Schloerb, F. P.; Ten
Brummelaar, T.; McAlister, H.; Ridgway, S.; Sturmann, L.; Sturmann, J.; Turner, N.; Baron, F.; Kraus, S.; Tannirkulam, A.; Williams, P. M. (2011). "First Visual Orbit for the Prototypical
997:
of the stars that orbit one another in WR 140 may be responsible for concentrating dust into discrete bands, it is not known how the concentric shells are formed. It is thought that nuclear processes in the WolfâRayet star may contribute an unusual degree of coherence to dust emissions.
1039:, which then carries it away from the star at several hundred kilometers per second. It is not well understood whether the unusual concentricity of WR 140's dust is due to interactions between the two stellar winds or is the result of nuclear processes in the WolfâRayet member.
919:, although WR 133 also in Cygnus is comparably bright. Being less massive, less luminous, and probably less visually bright than its primary the WolfâRayet component is identified as the secondary star, despite the fact that it dominates the spectrum with its broad
1043:
helium burning and another. This period is close to eight years, with new emissions having been observed in 1985, 1993, 2001, and 2009. One estimate places the distance between shells at around 1.4 trillion km, meaning that if the
832:
production. In this mode of cosmic dust production, detritus enriched in silicon and carbon is periodically blown into the wider universe by certain stars toward the end of their lives. Such stars are termed WolfâRayets.
961:, whose visual brightness varies only very slightly. Interest with this WR 140 system is principally observing the infrared light fluctuations during the component's orbit, being extensively studied because of its episodic
2638:
1396:
Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits".
1020:
This collapse eventually began to slow as it grew more intense and heated the star's interior. Along the edge of the core a thin shell experienced temperatures and pressures sufficient to begin
3960:
3643:
1269:
M.; Marsh, Kenneth A.; McCallon, Howard L.; Schneider, Stephen E.; Stiening, Rae; Sykes, Matthew J.; Weinberg, Martin D.; Wheaton, William A.; Wheelock, Sherry L.; Zacarias, N. (2003).
4023:
1996:
1752:
Pittard, J. M.; Pollock, A. M. T.; Rauw, G.; Reinecke, N.; Ribeiro, J.; Romeo, N.; SĂĄnchez-Gallego, J. R.; Dos Santos, E. M.; Schanne, L.; et al. (2011).
1714:
Panov, Kiril P.; Altmann, Martin; Seggewiss, Wilhelm (March 2000). "Long-term photometry of the Wolf-Rayet stars WR 137, WR 140, WR 148, and WR 153".
740:
4013:
939:
absorption lines of the O4â5 primary and C IV emission lines at 465.0 nm for WR 140. Separation between these two stars varies from 1.3
1300:
Van Der Hucht, K. A. (2006). "New
Galactic WolfâRayet stars, and candidates. An annex to the VIIth Catalogue of Galactic WolfâRayet Stars".
1989:
1356:
Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data
Catalog: General Catalogue of Variable Stars (Samus+, 2007-2017)".
935:
of 7.9 ± 0.2 years, which has been determined from the velocity variations observed with the component's spectral lines, mostly from the
958:
1593:"Orbital Elements and Individual Component Masses from Joint Spectroscopic and Astrometric Data of Double-line Spectroscopic Binaries"
36:, taken in July 2022. The nebula is formed by the binary and only the innermost shells were previously imaged with Keck in 1999/2001.
2610:
4028:
4018:
3998:
1982:
51:
1076:
Monnier, J. D.; Tuthill, P. G.; Danchi, W. C. (2002-03-01). "Proper
Motions of New Dust in the Colliding Wind Binary WR 140".
1027:
However, at the surface this loss of internal radiation pressure had the effect of blowing the outermost layers of the star's
744:
4003:
864:
radiation, the wavelength of its greatest luminosity. This has the effect of rebroadcasting the star's UV radiation in the
916:
1225:
Shenavrin, V. I.; Taranova, O. G.; Nadzhip, A. E. (2011). "Search for and study of hot circumstellar dust envelopes".
1467:
4033:
1198:
Ducati, J. R. (2002). "VizieR On-Line Data
Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".
1056:
869:
2371:
1454:
1017:. The WolfâRayet star began to lose volume as its own gravitational contraction compacted its cooler interior.
951:
720:
2926:
1508:
3620:
3330:
2016:
1059:
image at top right these intervals can be highly stable, continuing over many decades or hundreds of years.
885:
33:
4008:
2567:
2005:
1014:
805:
728:
491:
115:
66:
3515:
4038:
3571:
2534:
2203:
966:
698:
620:
437:
1858:
Taranova, O. G.; Shenavrin, V. I. (2011-01-01). "WR 140 (=V1687 Cyg): Infrared photometry, 2001â2010".
1754:"Spectroscopy of the archetype colliding-wind binary WR 140 during the 2009 January periastron passage"
3402:
1867:
1806:
1765:
1733:
1672:
1614:
1552:
1486:
1415:
1365:
1319:
1282:
1234:
1207:
1159:
1095:
1021:
785:
394:
267:
1013:
this fusion provided, the balance that determines the radii of all stars shifted decisively towards
781:
180:
120:
3220:
3505:
1951:
1910:
1891:
1723:
1632:
1604:
1568:
1542:
1476:
1431:
1405:
1335:
1309:
1250:
1175:
1149:
1119:
1085:
1035:
The cast-off materials are essentially extremely large injections of cosmic dust into the star's
1010:
901:
877:
865:
288:
142:
131:
98:
3533:
2035:
1883:
1111:
940:
881:
793:
736:
462:
44:
3455:
3450:
3432:
3190:
2524:
1961:
1875:
1814:
1773:
1737:
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1560:
1496:
1491:
1423:
1419:
1327:
1323:
1242:
1167:
1163:
1103:
980:
brightness increases dramatically and then slowly drops again over a period of months. Here
685:
607:
251:
1270:
769:
3523:
3320:
3170:
3100:
3095:
3090:
3055:
2976:
837:
370:
199:
74:
3120:
2519:
1871:
1810:
1769:
1676:
1618:
1556:
1369:
1286:
1238:
1211:
1099:
3973:
3968:
3407:
1052:
932:
724:
712:
517:
344:
259:
239:
227:
1591:
Anguita-Aguero, Jennifer; Mendez, Rene A.; ClaverĂa, RubĂ©n M.; Costa, Edgardo (2022).
1001:
As the WolfâRayet star in WR 140 neared the end of its short life its core ran out of
3992:
3460:
3070:
3065:
2158:
2063:
1895:
1778:
1753:
1636:
1564:
1435:
1339:
1254:
1123:
936:
920:
801:
216:
175:
61:
1572:
1179:
3886:
3881:
3876:
3871:
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3856:
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3248:
3209:
3180:
3135:
3130:
3085:
2183:
2178:
2098:
1036:
994:
981:
667:
640:
580:
1501:
1458:
1271:"VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)"
896:
3060:
1427:
1331:
1171:
3922:
3917:
3912:
3907:
3902:
3846:
3841:
3836:
3831:
3826:
3821:
3816:
3811:
3806:
3801:
3796:
3791:
3546:
3541:
3412:
3389:
3369:
3364:
3356:
3256:
3175:
3125:
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2514:
2509:
2504:
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2489:
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2148:
2093:
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1028:
962:
904:
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861:
829:
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413:
165:
154:
124:
87:
1627:
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3711:
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1246:
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973:
928:
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647:
600:
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459:
274:
187:
1966:
1939:
1887:
1115:
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2711:
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2701:
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2585:
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2547:
2542:
2494:
2173:
2168:
2163:
2153:
2143:
2138:
2133:
2073:
1940:"The orbit and stellar masses of the archetype colliding-wind binary WR 140"
732:
1795:"Photometric variability of a complete sample of northern WolfâRayet stars"
1974:
1834:
1690:
931:. Its current accepted spectroscopic orbit is highly eccentric and has an
3932:
3651:
3615:
3589:
3584:
3579:
3500:
3495:
3490:
3485:
3480:
3475:
3470:
3440:
3397:
3306:
3301:
3296:
3291:
3286:
3281:
3105:
2661:
2656:
2651:
2444:
2439:
2434:
2429:
2424:
2419:
2414:
2409:
2404:
2361:
2356:
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2346:
2341:
2336:
2331:
2326:
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2316:
2311:
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2301:
2296:
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2276:
2271:
2266:
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2256:
2251:
2246:
2241:
2236:
2231:
2128:
2123:
2118:
2113:
2108:
2103:
1728:
1410:
1314:
1090:
1002:
977:
944:
845:
3951:
3937:
3927:
3422:
3417:
3374:
3266:
3185:
3160:
3155:
3115:
3110:
3009:
2646:
2628:
2479:
2399:
2394:
2389:
2384:
2379:
2226:
2221:
2216:
2211:
2193:
2188:
2048:
950:
WR 140 is listed as a WolfâRayet variable star, and has been given the
849:
54:
47:
1663:
Williams, Peredur (2011). "Results from the 2009 campaign on WR 140".
3605:
3562:
3347:
3150:
3145:
3034:
3029:
3024:
3019:
3004:
2999:
2994:
2989:
2984:
1512:
1140:
Van
Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".
1006:
857:
853:
841:
763:
705:
660:
627:
279:
1956:
1819:
1794:
1609:
1481:
1107:
3465:
3379:
3335:
3140:
2043:
1547:
1154:
915:
WR 140 has been described as the brightest WolfâRayet star in the
895:
809:
748:
316:
872:. The rebroadcast of the star's UV radiation by carbon and other
3761:
3261:
2026:
361:
243:
231:
27:
1978:
2851:
2806:
1463:
Data
Release 2: Summary of the contents and survey properties"
1044:
1032:
this cycle of intermittent helium fusion can repeat itself.
1047:
were such a WolfâRayet star one shell would be well into the
808:, lying in the sky at the centre of the triangle formed by
907:
for V1687 Cygni, plotted from data published by Panov
3959:
3950:
3895:
3642:
3633:
3598:
3570:
3561:
3532:
3514:
3431:
3388:
3355:
3346:
3319:
3247:
3219:
3208:
3043:
2975:
2637:
2609:
2566:
2533:
2370:
2202:
2034:
2025:
1665:
Bulletin de la Société Royale des
Sciences de LiĂšge
1055:before another shell were cast off. As seen in the
1457:; et al. (Gaia collaboration) (August 2018).
923:. The primary star is an O4â5 star, most likely a
828:WR 140 is thought to be a prototypical example of
1944:Monthly Notices of the Royal Astronomical Society
1758:Monthly Notices of the Royal Astronomical Society
32:This image shows WR 140 and its nebula with JWST
965:formation. It is now regarded as the prototype
1835:"Episodic (and variable) dust-making WR stars"
836:The outermost layers of a WolfâRayet star are
1990:
1911:"Surprised no-one spotted my awful maths yet"
92:+43° 51′ 16.2802″
8:
876:traveling away from its surface creates the
1658:
1656:
1654:
1652:
1650:
1648:
1646:
1275:CDS/ADC Collection of Electronic Catalogues
1200:CDS/ADC Collection of Electronic Catalogues
1135:
1133:
3956:
3639:
3567:
3352:
3216:
2031:
1997:
1983:
1975:
1527:
1525:
1523:
1521:
1965:
1955:
1818:
1777:
1727:
1626:
1608:
1586:
1584:
1582:
1546:
1500:
1490:
1480:
1409:
1313:
1153:
1089:
1193:
1191:
1189:
4024:Objects with variable star designations
1938:Thomas, Joshua D.; et al. (2021).
1793:Moffat, A. F. J.; Shara, M. M. (1986).
1068:
223:
1351:
1349:
18:
1449:
1447:
1445:
868:, and it is this that is detected by
7:
1391:
1389:
1387:
1385:
1383:
1381:
1379:
50:
993:While interactions between the two
959:General Catalogue of Variable Stars
860:. The heating is due to the star's
235:
16:Star in the constellation of Cygnus
14:
1535:The Astrophysical Journal Letters
1779:10.1111/j.1365-2966.2011.19035.x
884:rather than the far more common
780:is a visually moderately bright
26:
1533:Colliding-wind Binary WR 140".
1509:Gaia DR2 record for this source
976:passage every eight years, the
258:0.5815 ± 0.0286
4014:Henry Draper Catalogue objects
1:
892:Binary system characteristics
1468:Astronomy & Astrophysics
1051:and around 5% of the way to
989:Mechanism of dust production
943:at periastron to 23.9 AU at
1502:10.1051/0004-6361/201833051
792:, whose primary star is an
4055:
1716:Astronomy and Astrophysics
1565:10.1088/2041-8205/742/1/L1
1428:10.1051/0004-6361:20041213
1398:Astronomy and Astrophysics
1358:Vizier Online Data Catalog
1332:10.1051/0004-6361:20065819
1302:Astronomy and Astrophysics
1172:10.1051/0004-6361:20078357
1142:Astronomy and Astrophysics
2012:
1880:10.1134/S1063773710091014
1247:10.1134/S1063772911010070
1078:The Astrophysical Journal
952:variable star designation
756:
718:
711:
633:
573:
568:
315:
311:
193:
186:
109:
41:
24:
1628:10.3847/1538-3881/ac478c
1597:The Astronomical Journal
2017:List of stars in Cygnus
2006:Constellation of Cygnus
1738:2000A&A...355..607P
1492:2018A&A...616A...1G
1420:2004A&A...424..727P
1324:2006A&A...458..453V
1164:2007A&A...474..653V
1009:. With the loss of the
880:of a WolfâRayet: broad
800:. It is located in the
289:Absolute magnitude
143:Apparent magnitude
132:Apparent magnitude
99:Apparent magnitude
34:Mid-Infrared Instrument
4029:Durchmusterung objects
4019:Spectroscopic binaries
3999:Cygnus (constellation)
3621:ZTF J203349.8+322901.1
1967:10.1093/mnras/stab1181
1015:gravitational collapse
912:
492:Argument of periastron
967:colliding-wind binary
899:
438:Longitude of the node
3403:North America Nebula
1799:Astronomical Journal
1691:"WR140 Introduction"
786:spectroscopic binary
1872:2011AstL...37...30T
1811:1986AJ.....92..952M
1770:2011MNRAS.418....2F
1677:2011BSRSL..80..595W
1619:2022AJ....163..118A
1557:2011ApJ...742L...1M
1370:2009yCat....102025S
1287:2003yCat.2246....0C
1239:2011ARep...55...31S
1212:2002yCat.2237....0D
1100:2002ApJ...567L.137M
917:northern hemisphere
870:suitable telescopes
757:Database references
747: J20205+4351,
21:
3506:Soap Bubble Nebula
1909:Mark McCaughrean.
1011:radiation pressure
913:
886:absorption spectra
784:placed within the
751:J20202798+4351164
713:Other designations
238: â2.047
226: â4.653
176:Variable type
116:Spectral type
19:
4034:Hipparcos objects
3986:
3985:
3982:
3981:
3946:
3945:
3629:
3628:
3557:
3556:
3550:
3339:
3315:
3314:
3204:
3203:
1860:Astronomy Letters
1227:Astronomy Reports
775:
774:
278:(1,720 ± 80
273:5,600 ± 300
4046:
4004:WolfâRayet stars
3957:
3640:
3568:
3544:
3353:
3333:
3217:
2032:
1999:
1992:
1985:
1976:
1971:
1969:
1959:
1950:(4): 5221â5230.
1925:
1924:
1922:
1921:
1906:
1900:
1899:
1855:
1849:
1848:
1846:
1845:
1831:
1825:
1824:
1822:
1790:
1784:
1783:
1781:
1748:
1742:
1741:
1731:
1729:astro-ph/0002221
1711:
1705:
1704:
1702:
1701:
1687:
1681:
1680:
1660:
1641:
1640:
1630:
1612:
1588:
1577:
1576:
1550:
1529:
1516:
1506:
1504:
1494:
1484:
1451:
1440:
1439:
1413:
1411:astro-ph/0406573
1393:
1374:
1373:
1353:
1344:
1343:
1317:
1315:astro-ph/0609008
1297:
1291:
1290:
1265:
1259:
1258:
1222:
1216:
1215:
1195:
1184:
1183:
1157:
1137:
1128:
1127:
1093:
1091:astro-ph/0202315
1084:(2): L137âL140.
1073:
902:ultraviolet band
882:emission spectra
563:
562:
561:
536:
534:
510:
509:
508:
496:
484:
483:
482:
475:
467:
451:
449:
442:
429:
428:
427:
407:
405:
387:
386:
385:
375:
360:
359:
358:
307:: â6.11 to â5.94
237:
225:
110:Characteristics
102:
82:
77:
42:Observation data
30:
22:
4054:
4053:
4049:
4048:
4047:
4045:
4044:
4043:
3989:
3988:
3987:
3978:
3942:
3891:
3625:
3594:
3553:
3528:
3524:Crescent Nebula
3510:
3456:IRAS 20324+4057
3451:IRAS 19475+3119
3427:
3384:
3342:
3322:
3311:
3243:
3211:
3200:
3191:WISE J2000+3629
3101:GSC 03949-00967
3039:
2971:
2633:
2605:
2562:
2529:
2366:
2198:
2021:
2008:
2003:
1937:
1934:
1932:Further reading
1929:
1928:
1919:
1917:
1908:
1907:
1903:
1857:
1856:
1852:
1843:
1841:
1833:
1832:
1828:
1792:
1791:
1787:
1750:
1749:
1745:
1713:
1712:
1708:
1699:
1697:
1689:
1688:
1684:
1662:
1661:
1644:
1590:
1589:
1580:
1531:
1530:
1519:
1455:Brown, A. G. A.
1453:
1452:
1443:
1395:
1394:
1377:
1355:
1354:
1347:
1299:
1298:
1294:
1267:
1266:
1262:
1224:
1223:
1219:
1197:
1196:
1187:
1139:
1138:
1131:
1075:
1074:
1070:
1065:
991:
894:
826:
798:class O4â5 star
782:WolfâRayet star
752:
691:
688:
684:1,600,000
673:
670:
653:
650:
613:
610:
593:
590:
559:
557:
556:
554:
550:
548:
532:
530:
526:
524:
506:
504:
503:
501:
497:
489:
480:
478:
477:
473:
471:
457:
447:
445:
435:
425:
423:
422:
420:
403:
401:
383:
381:
380:
378:
371:Semi-major axis
368:
356:
354:
353:
351:
303:
294:
277:
234:
205:
200:Radial velocity
97:
80:
75:Right ascension
73:
43:
37:
31:
17:
12:
11:
5:
4052:
4050:
4042:
4041:
4036:
4031:
4026:
4021:
4016:
4011:
4006:
4001:
3991:
3990:
3984:
3983:
3980:
3979:
3977:
3976:
3971:
3965:
3963:
3954:
3948:
3947:
3944:
3943:
3941:
3940:
3935:
3930:
3925:
3920:
3915:
3910:
3905:
3899:
3897:
3893:
3892:
3890:
3889:
3884:
3879:
3874:
3869:
3864:
3859:
3854:
3849:
3844:
3839:
3834:
3829:
3824:
3819:
3814:
3809:
3804:
3799:
3794:
3789:
3784:
3779:
3774:
3769:
3764:
3759:
3754:
3749:
3744:
3739:
3734:
3729:
3724:
3719:
3714:
3709:
3704:
3699:
3694:
3689:
3684:
3679:
3674:
3669:
3664:
3659:
3654:
3648:
3646:
3637:
3631:
3630:
3627:
3626:
3624:
3623:
3618:
3613:
3608:
3602:
3600:
3596:
3595:
3593:
3592:
3587:
3582:
3576:
3574:
3565:
3559:
3558:
3555:
3554:
3552:
3551:
3538:
3536:
3530:
3529:
3527:
3526:
3520:
3518:
3512:
3511:
3509:
3508:
3503:
3498:
3493:
3488:
3483:
3478:
3473:
3468:
3463:
3458:
3453:
3448:
3443:
3437:
3435:
3429:
3428:
3426:
3425:
3420:
3415:
3410:
3408:Pelican Nebula
3405:
3400:
3394:
3392:
3386:
3385:
3383:
3382:
3377:
3372:
3367:
3361:
3359:
3350:
3344:
3343:
3341:
3340:
3327:
3325:
3317:
3316:
3313:
3312:
3310:
3309:
3304:
3299:
3294:
3289:
3284:
3279:
3274:
3269:
3264:
3259:
3253:
3251:
3245:
3244:
3242:
3241:
3236:
3231:
3225:
3223:
3214:
3206:
3205:
3202:
3201:
3199:
3198:
3193:
3188:
3183:
3178:
3173:
3171:PSR J2032+4127
3168:
3163:
3158:
3153:
3148:
3143:
3138:
3133:
3128:
3123:
3118:
3113:
3108:
3103:
3098:
3093:
3088:
3083:
3078:
3073:
3071:Cygnus OB2 #12
3068:
3066:Cygnus OB2 #8A
3063:
3058:
3053:
3047:
3045:
3041:
3040:
3038:
3037:
3032:
3027:
3022:
3017:
3012:
3007:
3002:
2997:
2992:
2987:
2981:
2979:
2973:
2972:
2970:
2969:
2964:
2959:
2954:
2949:
2944:
2939:
2934:
2929:
2924:
2919:
2914:
2909:
2904:
2899:
2894:
2889:
2884:
2879:
2874:
2869:
2864:
2859:
2854:
2849:
2844:
2839:
2834:
2829:
2824:
2819:
2814:
2809:
2804:
2799:
2794:
2789:
2784:
2779:
2774:
2769:
2764:
2759:
2754:
2749:
2744:
2739:
2734:
2729:
2724:
2719:
2714:
2709:
2704:
2699:
2694:
2689:
2684:
2679:
2674:
2669:
2664:
2659:
2654:
2649:
2643:
2641:
2635:
2634:
2632:
2631:
2626:
2621:
2615:
2613:
2607:
2606:
2604:
2603:
2598:
2593:
2588:
2583:
2578:
2572:
2570:
2564:
2563:
2561:
2560:
2555:
2550:
2545:
2539:
2537:
2531:
2530:
2528:
2527:
2522:
2517:
2512:
2507:
2502:
2497:
2492:
2487:
2482:
2477:
2472:
2467:
2462:
2457:
2452:
2447:
2442:
2437:
2432:
2427:
2422:
2417:
2412:
2407:
2402:
2397:
2392:
2387:
2382:
2376:
2374:
2368:
2367:
2365:
2364:
2359:
2354:
2349:
2344:
2339:
2334:
2329:
2324:
2319:
2314:
2309:
2304:
2299:
2294:
2289:
2284:
2279:
2274:
2269:
2264:
2259:
2254:
2249:
2244:
2239:
2234:
2229:
2224:
2219:
2214:
2208:
2206:
2200:
2199:
2197:
2196:
2191:
2186:
2181:
2176:
2171:
2166:
2161:
2156:
2151:
2146:
2141:
2136:
2134:Ï (Azelfafage)
2131:
2126:
2121:
2116:
2111:
2106:
2101:
2096:
2091:
2086:
2081:
2076:
2071:
2066:
2061:
2056:
2051:
2046:
2040:
2038:
2029:
2023:
2022:
2020:
2019:
2013:
2010:
2009:
2004:
2002:
2001:
1994:
1987:
1979:
1973:
1972:
1933:
1930:
1927:
1926:
1901:
1850:
1826:
1820:10.1086/114227
1785:
1743:
1706:
1682:
1642:
1578:
1517:
1441:
1404:(2): 727â732.
1375:
1345:
1308:(2): 453â459.
1292:
1260:
1217:
1185:
1148:(2): 653â664.
1129:
1108:10.1086/340005
1067:
1066:
1064:
1061:
1053:Alpha Centauri
990:
987:
972:Shortly after
933:orbital period
921:emission lines
893:
890:
825:
822:
773:
772:
767:
759:
758:
754:
753:
735: 100287,
731: 193793,
719:
716:
715:
709:
708:
702:
694:
693:
689:
686:
682:
676:
675:
671:
668:
664:
656:
655:
651:
648:
644:
636:
635:
631:
630:
624:
616:
615:
611:
608:
604:
596:
595:
591:
588:
584:
576:
575:
571:
570:
566:
565:
552:
546:
543:Semi-amplitude
539:
538:
528:
522:
518:Semi-amplitude
513:
512:
499:
486:
485:
468:
454:
453:
443:
432:
431:
418:
409:
408:
399:
390:
389:
376:
365:
364:
349:
340:
339:
336:
330:
329:
326:
320:
319:
313:
312:
309:
308:
302:: â6.6 to â4.8
297:
292:
284:
283:
271:
263:
262:
256:
247:
246:
221:
212:
211:
210:3.10 km/s
208:
203:
195:
194:
191:
190:
184:
183:
178:
172:
171:
168:
161:
160:
157:
150:
149:
146:
139:
138:
135:
128:
127:
118:
112:
111:
107:
106:
103:
94:
93:
90:
84:
83:
81:20 20 27.97608
78:
70:
69:
64:
58:
57:
39:
38:
25:
15:
13:
10:
9:
6:
4:
3:
2:
4051:
4040:
4037:
4035:
4032:
4030:
4027:
4025:
4022:
4020:
4017:
4015:
4012:
4010:
4009:2MASS objects
4007:
4005:
4002:
4000:
3997:
3996:
3994:
3975:
3972:
3970:
3967:
3966:
3964:
3962:
3958:
3955:
3953:
3949:
3939:
3936:
3934:
3931:
3929:
3926:
3924:
3921:
3919:
3916:
3914:
3911:
3909:
3906:
3904:
3901:
3900:
3898:
3894:
3888:
3885:
3883:
3880:
3878:
3875:
3873:
3870:
3868:
3865:
3863:
3860:
3858:
3855:
3853:
3850:
3848:
3845:
3843:
3840:
3838:
3835:
3833:
3830:
3828:
3825:
3823:
3820:
3818:
3815:
3813:
3810:
3808:
3805:
3803:
3800:
3798:
3795:
3793:
3790:
3788:
3785:
3783:
3780:
3778:
3775:
3773:
3770:
3768:
3765:
3763:
3760:
3758:
3755:
3753:
3750:
3748:
3745:
3743:
3740:
3738:
3735:
3733:
3730:
3728:
3725:
3723:
3720:
3718:
3715:
3713:
3710:
3708:
3705:
3703:
3700:
3698:
3695:
3693:
3690:
3688:
3685:
3683:
3680:
3678:
3675:
3673:
3670:
3668:
3665:
3663:
3660:
3658:
3655:
3653:
3650:
3649:
3647:
3645:
3641:
3638:
3636:
3632:
3622:
3619:
3617:
3614:
3612:
3609:
3607:
3604:
3603:
3601:
3597:
3591:
3588:
3586:
3583:
3581:
3578:
3577:
3575:
3573:
3569:
3566:
3564:
3560:
3548:
3543:
3540:
3539:
3537:
3535:
3531:
3525:
3522:
3521:
3519:
3517:
3513:
3507:
3504:
3502:
3499:
3497:
3494:
3492:
3489:
3487:
3484:
3482:
3479:
3477:
3474:
3472:
3469:
3467:
3464:
3462:
3461:Kronberger 61
3459:
3457:
3454:
3452:
3449:
3447:
3444:
3442:
3439:
3438:
3436:
3434:
3430:
3424:
3421:
3419:
3416:
3414:
3411:
3409:
3406:
3404:
3401:
3399:
3396:
3395:
3393:
3391:
3387:
3381:
3378:
3376:
3373:
3371:
3368:
3366:
3363:
3362:
3360:
3358:
3354:
3351:
3349:
3345:
3337:
3332:
3329:
3328:
3326:
3324:
3318:
3308:
3305:
3303:
3300:
3298:
3295:
3293:
3290:
3288:
3285:
3283:
3280:
3278:
3275:
3273:
3270:
3268:
3265:
3263:
3260:
3258:
3255:
3254:
3252:
3250:
3246:
3240:
3237:
3235:
3232:
3230:
3227:
3226:
3224:
3222:
3218:
3215:
3213:
3207:
3197:
3194:
3192:
3189:
3187:
3184:
3182:
3179:
3177:
3174:
3172:
3169:
3167:
3164:
3162:
3159:
3157:
3154:
3152:
3149:
3147:
3144:
3142:
3139:
3137:
3134:
3132:
3129:
3127:
3124:
3122:
3119:
3117:
3114:
3112:
3109:
3107:
3104:
3102:
3099:
3097:
3094:
3092:
3089:
3087:
3084:
3082:
3079:
3077:
3074:
3072:
3069:
3067:
3064:
3062:
3059:
3057:
3054:
3052:
3049:
3048:
3046:
3042:
3036:
3033:
3031:
3028:
3026:
3023:
3021:
3018:
3016:
3013:
3011:
3008:
3006:
3003:
3001:
2998:
2996:
2993:
2991:
2988:
2986:
2983:
2982:
2980:
2978:
2974:
2968:
2965:
2963:
2960:
2958:
2955:
2953:
2950:
2948:
2945:
2943:
2940:
2938:
2935:
2933:
2930:
2928:
2925:
2923:
2920:
2918:
2915:
2913:
2910:
2908:
2905:
2903:
2900:
2898:
2895:
2893:
2890:
2888:
2885:
2883:
2880:
2878:
2875:
2873:
2870:
2868:
2865:
2863:
2860:
2858:
2855:
2853:
2850:
2848:
2845:
2843:
2840:
2838:
2835:
2833:
2830:
2828:
2825:
2823:
2820:
2818:
2815:
2813:
2810:
2808:
2805:
2803:
2800:
2798:
2795:
2793:
2790:
2788:
2785:
2783:
2780:
2778:
2775:
2773:
2770:
2768:
2765:
2763:
2760:
2758:
2755:
2753:
2750:
2748:
2745:
2743:
2740:
2738:
2735:
2733:
2730:
2728:
2725:
2723:
2720:
2718:
2715:
2713:
2710:
2708:
2705:
2703:
2700:
2698:
2695:
2693:
2690:
2688:
2685:
2683:
2680:
2678:
2675:
2673:
2670:
2668:
2665:
2663:
2660:
2658:
2655:
2653:
2650:
2648:
2645:
2644:
2642:
2640:
2636:
2630:
2627:
2625:
2622:
2620:
2617:
2616:
2614:
2612:
2608:
2602:
2599:
2597:
2594:
2592:
2589:
2587:
2584:
2582:
2579:
2577:
2574:
2573:
2571:
2569:
2565:
2559:
2556:
2554:
2551:
2549:
2546:
2544:
2541:
2540:
2538:
2536:
2532:
2526:
2523:
2521:
2518:
2516:
2513:
2511:
2508:
2506:
2503:
2501:
2498:
2496:
2493:
2491:
2488:
2486:
2483:
2481:
2478:
2476:
2473:
2471:
2468:
2466:
2463:
2461:
2458:
2456:
2453:
2451:
2448:
2446:
2443:
2441:
2438:
2436:
2433:
2431:
2428:
2426:
2423:
2421:
2418:
2416:
2413:
2411:
2408:
2406:
2403:
2401:
2398:
2396:
2393:
2391:
2388:
2386:
2383:
2381:
2378:
2377:
2375:
2373:
2369:
2363:
2360:
2358:
2355:
2353:
2350:
2348:
2345:
2343:
2340:
2338:
2335:
2333:
2330:
2328:
2325:
2323:
2320:
2318:
2315:
2313:
2310:
2308:
2305:
2303:
2300:
2298:
2295:
2293:
2290:
2288:
2285:
2283:
2280:
2278:
2275:
2273:
2270:
2268:
2265:
2263:
2260:
2258:
2255:
2253:
2250:
2248:
2245:
2243:
2240:
2238:
2235:
2233:
2230:
2228:
2225:
2223:
2220:
2218:
2215:
2213:
2210:
2209:
2207:
2205:
2201:
2195:
2192:
2190:
2187:
2185:
2182:
2180:
2177:
2175:
2172:
2170:
2167:
2165:
2162:
2160:
2157:
2155:
2152:
2150:
2147:
2145:
2142:
2140:
2137:
2135:
2132:
2130:
2127:
2125:
2122:
2120:
2117:
2115:
2112:
2110:
2107:
2105:
2102:
2100:
2097:
2095:
2092:
2090:
2087:
2085:
2082:
2080:
2077:
2075:
2072:
2070:
2067:
2065:
2062:
2060:
2057:
2055:
2052:
2050:
2047:
2045:
2042:
2041:
2039:
2037:
2033:
2030:
2028:
2024:
2018:
2015:
2014:
2011:
2007:
2000:
1995:
1993:
1988:
1986:
1981:
1980:
1977:
1968:
1963:
1958:
1953:
1949:
1945:
1941:
1936:
1935:
1931:
1916:
1912:
1905:
1902:
1897:
1893:
1889:
1885:
1881:
1877:
1873:
1869:
1865:
1861:
1854:
1851:
1840:
1839:www.roe.ac.uk
1836:
1830:
1827:
1821:
1816:
1812:
1808:
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1796:
1789:
1786:
1780:
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1763:
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1730:
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1717:
1710:
1707:
1696:
1695:www.roe.ac.uk
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1437:
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1371:
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1359:
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1346:
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1316:
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1296:
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1276:
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1256:
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1240:
1236:
1232:
1228:
1221:
1218:
1213:
1209:
1205:
1201:
1194:
1192:
1190:
1186:
1181:
1177:
1173:
1169:
1165:
1161:
1156:
1151:
1147:
1143:
1136:
1134:
1130:
1125:
1121:
1117:
1113:
1109:
1105:
1101:
1097:
1092:
1087:
1083:
1079:
1072:
1069:
1062:
1060:
1058:
1054:
1050:
1046:
1040:
1038:
1033:
1030:
1025:
1023:
1022:helium fusion
1018:
1016:
1012:
1008:
1005:to fuse into
1004:
999:
996:
995:stellar winds
988:
986:
983:
982:stellar winds
979:
975:
970:
968:
964:
960:
956:
953:
948:
946:
942:
938:
934:
930:
926:
922:
918:
910:
906:
903:
898:
891:
889:
887:
883:
879:
875:
871:
867:
863:
859:
855:
851:
847:
843:
839:
834:
831:
823:
821:
819:
815:
811:
807:
803:
802:constellation
799:
795:
791:
787:
783:
779:
771:
768:
766:
765:
761:
760:
755:
750:
746:
742:
739:3164-1678-1,
738:
734:
730:
726:
723: Cygni,
722:
717:
714:
710:
707:
703:
701:
700:
696:
695:
692:
683:
681:
678:
677:
674:
665:
663:
662:
658:
657:
654:
645:
643:
642:
638:
637:
632:
629:
625:
623:
622:
618:
617:
614:
606:537,000
605:
603:
602:
598:
597:
594:
585:
583:
582:
578:
577:
572:
567:
553:
544:
541:
540:
529:
520:
519:
515:
514:
500:
495:
493:
488:
487:
469:
466:
464:
461:
456:
455:
444:
441:
439:
434:
433:
419:
417:
415:
411:
410:
400:
398:
396:
392:
391:
377:
374:
372:
367:
366:
363:
350:
348:
346:
342:
341:
337:
335:
332:
331:
327:
325:
322:
321:
318:
314:
310:
306:
301:
298:
296:
290:
286:
285:
281:
276:
272:
270:
269:
265:
264:
261:
257:
255:
253:
249:
248:
245:
241:
233:
229:
222:
220:
218:
217:Proper motion
214:
213:
209:
207:
201:
197:
196:
192:
189:
185:
182:
179:
177:
174:
173:
169:
167:
163:
162:
158:
156:
152:
151:
147:
144:
141:
140:
136:
133:
130:
129:
126:
122:
119:
117:
114:
113:
108:
104:
100:
96:
95:
91:
89:
86:
85:
79:
76:
72:
71:
68:
65:
63:
62:Constellation
60:
59:
56:
53:
49:
46:
40:
35:
29:
23:
4039:O-type stars
3181:W75N(B)-VLA2
3136:KIC 11145123
3131:KIC 11026764
3014:
1947:
1943:
1918:. Retrieved
1914:
1904:
1866:(1): 30â39.
1863:
1859:
1853:
1842:. Retrieved
1838:
1829:
1802:
1798:
1788:
1761:
1757:
1746:
1719:
1715:
1709:
1698:. Retrieved
1694:
1685:
1668:
1664:
1600:
1596:
1538:
1534:
1472:
1466:
1460:
1401:
1397:
1361:
1357:
1305:
1301:
1295:
1278:
1274:
1263:
1233:(1): 31â81.
1230:
1226:
1220:
1203:
1199:
1145:
1141:
1081:
1077:
1071:
1041:
1037:stellar wind
1034:
1026:
1019:
1000:
992:
971:
954:
949:
914:
908:
835:
827:
824:Significance
789:
777:
776:
762:
743: 1232,
704:35,000
697:
679:
659:
639:
626:70,000
619:
599:
579:
542:
516:
490:
458:
436:
412:
395:Eccentricity
393:
369:
343:
333:
323:
304:
299:
287:
266:
250:
215:
198:
3923:HD 191806 b
3913:HD 187123 b
3908:HD 185269 b
3547:Veil Nebula
3545:(including
3542:Cygnus Loop
3413:Sadr Region
3370:Barnard 147
3365:Barnard 146
3334:(including
3257:Berkeley 86
3221:Association
3176:SPECULOOS-3
3126:KIC 9832227
3121:KIC 8462852
3086:G79.29+0.46
3056:BD+40° 4210
2064:Δ (Aljanah)
2059:ÎŽ (Fawaris)
2049:ÎČ (Albireo)
1764:(1): 2â13.
1722:: 607â616.
1029:photosphere
905:light curve
830:cosmic dust
699:Temperature
621:Temperature
551:(secondary)
414:Inclination
166:color index
155:color index
88:Declination
3993:Categories
3762:64b (PH1b)
3635:Exoplanets
3446:Egg Nebula
3277:Messier 39
3272:Messier 29
3239:Cygnus OB9
3234:Cygnus OB7
3229:Cygnus OB2
3081:Cygnus X-3
3076:Cygnus X-1
3061:BD+43 3654
1957:2101.10563
1920:2022-09-02
1844:2022-09-02
1700:2022-08-29
1610:2201.04134
1603:(3): 118.
1482:1804.09365
1281:: II/246.
1063:References
1049:Oort Cloud
974:periastron
929:supergiant
727:+43°3571,
680:Luminosity
646:20.5
601:Luminosity
460:Periastron
188:Astrometry
145: (K)
134: (J)
3903:b Cygni b
3611:4C +48.48
3433:Planetary
3321:Molecular
3196:Wolf 1069
3166:N6946-BH1
3051:AFGL 2591
2204:Flamsteed
2044:α (Deneb)
1896:121357413
1888:0320-0108
1637:245854028
1548:1111.1266
1541:(1): L1.
1436:119387088
1340:119104786
1255:122700080
1155:0708.1752
1124:119363464
1116:0004-637X
955:V1687 Cyg
878:signature
796:spectral
790:SBC9 1232
586:8.4
527:(primary)
498:(primary)
334:Companion
101: (V)
3952:Exomoons
3933:KELT-20b
3616:Cygnus A
3563:Galaxies
3501:NGC 7048
3496:NGC 7027
3491:NGC 7026
3486:NGC 7008
3481:NGC 6884
3476:NGC 6881
3471:NGC 6826
3441:Abell 78
3398:NGC 6914
3331:Cygnus X
3307:NGC 6910
3302:NGC 6871
3297:NGC 6866
3292:NGC 6834
3287:NGC 6819
3282:NGC 6811
3212:clusters
3106:HAT-P-17
3096:G 208-45
3091:G 208-44
2852:86 (PH2)
2807:64 (PH1)
2372:Variable
2054:Îł (Sadr)
1573:17402120
1180:18759600
1003:hydrogen
978:infrared
945:apastron
866:infrared
846:nitrogen
838:enriched
690:☉
672:☉
666:35
652:☉
612:☉
592:☉
291: (M
268:Distance
252:Parallax
3974:1708b I
3969:1625b I
3938:TrES-5b
3928:KELT-9b
3423:Sh2-106
3418:Sh2-101
3375:IC 5146
3348:Nebulae
3267:IC 5146
3186:WASP-48
3161:MWC 349
3156:KOI-256
3116:KELT-20
1915:Twitter
1868:Bibcode
1807:Bibcode
1805:: 952.
1766:Bibcode
1734:Bibcode
1673:Bibcode
1671:: 595.
1615:Bibcode
1553:Bibcode
1487:Bibcode
1416:Bibcode
1366:Bibcode
1320:Bibcode
1283:Bibcode
1235:Bibcode
1208:Bibcode
1160:Bibcode
1096:Bibcode
957:in the
850:silicon
818:ÎŽ Cygni
814:Îł Cygni
794:evolved
569:Details
481:â0.0039
479:+0.0036
357:â0.0035
355:+0.0037
324:Primary
55:J2000.0
52:Equinox
48:J2000.0
20:WR 140
3961:Kepler
3644:Kepler
3606:3C 438
3323:clouds
3151:KOI-81
3146:KOI-74
3111:KELT-9
2639:Kepler
2611:Gliese
2601:197037
2596:191806
2591:188753
2586:187123
2581:185435
2576:185269
2347:71 (g)
2342:68 (A)
2337:63 (f)
2327:59 (f)
2277:29 (b)
2272:28 (b)
2267:27 (b)
2262:26 (e)
2247:20 (d)
2237:16 (c)
1894:
1886:
1635:
1571:
1513:VizieR
1475:. A1.
1434:
1338:
1253:
1178:
1122:
1114:
1007:helium
937:Balmer
911:(2000)
909:et al.
874:metals
854:carbon
842:oxygen
806:Cygnus
788:star,
778:WR 140
764:SIMBAD
661:Radius
511:°
452:°
430:°
406:0.0034
402:0.9012
352:7.9241
345:Period
170:+0.40
159:â0.35
148:5.037
137:5.547
67:Cygnus
3896:Other
3887:1708b
3877:1649b
3872:1658b
3867:1652b
3862:1625b
3857:1520b
3852:1229b
3599:Other
3466:M1-92
3380:L1014
3336:DR 21
3141:KOI-5
3044:Other
2525:V2513
2520:V2214
2515:V1974
2510:V1794
2505:V1668
2500:V1500
2495:V1489
2490:V1334
2485:V1191
2480:V1143
2475:V1057
2470:V1027
2036:Bayer
2027:Stars
1952:arXiv
1892:S2CID
1724:arXiv
1633:S2CID
1605:arXiv
1569:S2CID
1543:arXiv
1507:
1477:arXiv
1432:S2CID
1406:arXiv
1336:S2CID
1310:arXiv
1251:S2CID
1176:S2CID
1150:arXiv
1120:S2CID
1086:arXiv
925:giant
810:Deneb
749:2MASS
721:V1687
507:â0.68
505:+0.70
502:42.31
476:.1825
463:epoch
446:349.1
421:119.4
384:â0.23
382:+0.22
317:Orbit
236:Dec.:
105:6.85
45:Epoch
3847:737b
3842:560b
3837:452b
3832:451b
3827:432b
3822:419b
3817:409b
3807:371b
3792:186b
3590:7013
3585:6946
3580:6801
3390:H II
3357:Dark
3262:DR 6
3249:Open
3210:Star
3010:138a
2967:1708
2962:1649
2957:1625
2952:1520
2947:1229
2629:1245
2558:8193
2553:7912
2548:7767
2543:7633
2465:V476
2460:V404
2455:V389
2450:V380
1884:ISSN
1461:Gaia
1279:2246
1204:2237
1112:ISSN
1057:JWST
963:dust
852:and
816:and
770:data
741:SBC9
641:Mass
581:Mass
564:km/s
560:â1.1
558:+1.2
555:68.5
537:km/s
531:29.3
470:MJD
426:â3.4
424:+3.7
379:8.30
164:BâV
153:UâB
121:WC7p
3787:87c
3782:78b
3777:70b
3772:69b
3767:68b
3757:61b
3752:56b
3747:47b
3742:41b
3737:40b
3732:39b
3727:36b
3722:34b
3717:33b
3712:32b
3707:28b
3702:23b
3697:22b
3692:17b
3687:16b
3682:15b
3677:11b
3572:NGC
3534:SNR
3035:150
3030:148
3025:147
3020:142
3015:140
3005:137
3000:136
2995:135
2990:134
2985:133
2942:737
2937:560
2932:452
2927:451
2922:445
2917:432
2912:419
2907:411
2902:385
2897:371
2892:289
2887:223
2882:186
2877:182
2872:167
2867:107
2624:806
2619:777
1962:doi
1948:504
1876:doi
1815:doi
1774:doi
1762:418
1720:355
1623:doi
1601:163
1561:doi
1539:742
1511:at
1497:doi
1473:616
1424:doi
1402:424
1328:doi
1306:458
1243:doi
1168:doi
1146:474
1104:doi
1082:567
1045:Sun
969:.
947:.
927:or
900:An
840:in
804:of
745:WDS
737:TYC
733:HIP
535:1.8
494:(Ï)
474:993
465:(T)
450:2.5
440:(Ω)
416:(i)
397:(e)
373:(a)
347:(P)
260:mas
254:(Ï)
240:mas
228:mas
224:RA:
219:(Ό)
3995::
3672:6b
3667:5b
3662:3c
3657:3b
3652:2b
3516:WR
2977:WR
2862:89
2857:87
2847:84
2842:80
2837:78
2832:70
2827:69
2822:68
2817:67
2812:66
2802:63
2797:61
2792:56
2787:51
2782:47
2777:45
2772:44
2767:43
2762:42
2757:41
2752:40
2747:39
2742:36
2737:35
2732:34
2727:33
2722:32
2717:31
2712:29
2707:28
2702:27
2697:23
2692:22
2687:18
2682:17
2677:16
2672:15
2667:11
2568:HD
2535:HR
2445:KY
2440:CH
2435:BI
2430:BC
2425:AZ
2420:TT
2415:SU
2410:SS
2405:RW
2362:75
2357:74
2352:72
2332:61
2322:57
2317:56
2312:55
2307:52
2302:47
2297:41
2292:39
2287:35
2282:33
2257:23
2252:22
2242:17
2232:15
1960:.
1946:.
1942:.
1913:.
1890:.
1882:.
1874:.
1864:37
1862:.
1837:.
1813:.
1803:92
1801:.
1797:.
1772:.
1760:.
1756:.
1732:.
1718:.
1693:.
1669:80
1667:.
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1631:.
1621:.
1613:.
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1485:.
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1102:.
1094:.
1080:.
941:AU
888:.
862:UV
848:,
844:,
820:.
812:,
729:HD
725:BD
574:WR
545:(K
521:(K
362:yr
338:WR
300:WR
280:pc
275:ly
244:yr
232:yr
202:(R
181:WR
125:O5
123:+
3918:c
3882:c
3812:c
3802:f
3797:e
3549:)
3338:)
2662:6
2657:5
2652:3
2647:2
2400:Y
2395:X
2390:W
2385:T
2380:R
2227:9
2222:8
2217:4
2212:2
2194:Q
2189:P
2184:Ï
2179:Ï
2174:Ï
2169:Ï
2164:Ï
2159:Ï
2154:Ï
2149:Ï
2144:Ï
2139:Ï
2129:Îż
2124:o
2119:o
2114:Ο
2109:Μ
2104:Ό
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295:)
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282:)
242:/
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204:v
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