731:, luminosity, and spectrum all classify it as an LBV. It shows brightness variations of a few tenths of a magnitude, but these do not seem to be associated with colour changes that would be expected from an LBV. The spectral type has varied slightly since its discovery, but not to the extent that would be normal for an LBV. If the lower Gaia DR2 distance were correct then the properties of Cygnus OB2 #12 would mean it would be expected to pulsate at low amplitude with a period of a few days.
552:
640:, which was inconsistent with the distance of other Cygnus OB2 members. However, the result included a significant amount of noise suggesting that it may have been inaccurate. Earlier measures of the parallax were too imprecise to be meaningful. If the closer distance were accepted then the star would be a more conventional blue supergiant with a luminosity around 440,000
54:
709:
47:
586:) away in Cygnus, and resides in a region of the Milky Way from which visible light is heavily absorbed by interstellar dust when viewed from Earth. The dust causes the star to be strongly reddened despite being an intrinsically hot and blue star, hence it has been extensively studied in the infra-red. Were it not for the dust
536:. This makes the star nearly two million times more luminous than the Sun, although estimates were even higher when the star was first discovered. It is now known to be a binary, with the companion approximately a tenth as bright. A very approximate initial estimate of the orbit gives the total system mass as 120
956:
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
850:; Herrero, A.; Jao, W.-C.; Mason, B. D.; Massey, P.; Moffat, A. F. J.; Walborn, N. R. (2014). "A High Angular Resolution Survey of Massive Stars in Cygnus OB2: Results from the Hubble Space Telescope Fine Guidance Sensors".
2152:
3474:
3157:
957:
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).
28:
605:
B star in a 100–200 year orbit. It is 2.3 magnitudes fainter than the primary star and 0.063" away. The other is 4.8 magnitudes fainter and about an arc-second distant. No
601:
There are several fainter stars around Cygnus OB2 #12, thought to comprise a small cluster. Two stars are only resolved by speckle interferometry. One is thought to be a
1510:
1473:
1417:
Chentsov, E. L.; Klochkova, V. G.; Panchuk, V. E.; Yushkin, M. V.; Nasonov, D. S. (2013). "Spectroscopy of 13 high-mass stars in the Cyg OB2 association".
1114:
Clark, J. S.; Najarro, F.; Negueruela, I.; Ritchie, B. W.; Urbaneja, M. A.; Howarth, I. D. (2012). "On the nature of the galactic early-B hypergiants".
480:
1231:
Nazé, Yaël; Rauw, Gregor; Czesla, Stefan; Mahy, Laurent; Campos, Fran (2019). "Variations on a theme: The puzzling behaviour of
Schulte 12".
1503:
1048:"On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary"
675:
However using the distance provided by Gaia EDR3 it was determined in one work that the star has a luminosity of only about 316,000
1396:
Klochkova, V. G.; Islentieva, E. S.; Panchuk, V. E. (2023-01-01). "On the status of the star
Schulte 12 in the association Cyg OB2".
672:, more consistent with estimates of the distance to Cygnus OB2, although there is still a significant amount of astrometric noise.
1167:
Maryeva, O. V.; Chentsov, E. L.; Goranskij, V. P.; Dyachenko, V. V.; Karpov, S. V.; Malogolovets, E. V.; Rastegaev, D. A. (2016).
3522:
2124:
3512:
1496:
75:
1046:
Oskinova, L. M.; Huenemoerder, D. P.; Hamann, W. -R.; Shenar, T.; Sander, A. A. C.; Ignace, R.; Todt, H.; Hainich, R. (2017).
712:
3537:
594:(Alpha Cygni), but because of the dust the observed visual magnitude is 11.4 so that it requires binoculars or a small
3527:
529:
3517:
740:
1885:
988:
Klochkova, V. G.; Chentsov, E. L. (2004). "The
Optical Spectrum of an LBV Candidate in the Cyg OB2 Association".
826:
2440:
697:
3134:
2844:
1530:
3532:
2081:
1519:
724:
587:
137:
88:
3029:
3085:
2048:
1717:
618:
427:
2916:
1436:
1362:
1307:
1250:
1190:
1133:
1069:
1007:
970:
923:
869:
798:
606:
525:
316:
551:
2734:
665:
630:
488:
484:
472:
3019:
1452:
1426:
1397:
1378:
1352:
1325:
1297:
1266:
1240:
1208:
1180:
1149:
1123:
1087:
1059:
1023:
997:
885:
859:
816:
788:
716:
337:
191:
180:
169:
158:
147:
120:
509:
3047:
1549:
442:
71:
2969:
2964:
2946:
2704:
2038:
1444:
1370:
1366:
1315:
1258:
1254:
1198:
1141:
1137:
1077:
1015:
931:
877:
806:
802:
610:
568:
414:
300:
958:
3037:
2834:
2684:
2614:
2609:
2604:
2569:
2490:
1483:
617:
emission suggests that there may be a hot luminous companion in a close orbit, with their
248:
96:
2634:
2033:
1440:
1311:
1194:
1073:
1011:
974:
927:
873:
3487:
3482:
2921:
847:
460:
308:
288:
276:
3506:
2974:
2579:
1672:
1577:
1456:
1329:
1270:
1212:
1091:
881:
820:
602:
265:
224:
83:
53:
1382:
1153:
1027:
889:
3400:
3395:
3390:
3385:
3380:
3375:
3370:
3365:
2762:
2723:
2694:
2649:
2644:
2599:
1697:
1692:
1612:
556:
394:
367:
1262:
1145:
959:"VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)"
811:
772:
2574:
1374:
3436:
3431:
3426:
3421:
3416:
3360:
3355:
3350:
3345:
3340:
3335:
3330:
3325:
3320:
3315:
3310:
3305:
3060:
3055:
2926:
2903:
2883:
2878:
2870:
2770:
2689:
2639:
2480:
2475:
2470:
2465:
2460:
2028:
2023:
2018:
2013:
2003:
1998:
1988:
1983:
1662:
1607:
1602:
1597:
1592:
1572:
1567:
1284:
Berlanas, S. R.; Wright, N. J.; Herrero, A.; Drew, J. E.; Lennon, D. J. (2019).
214:
203:
109:
24:
1082:
1047:
3300:
3295:
3290:
3285:
3280:
3270:
3265:
3260:
3255:
3250:
3245:
3240:
3235:
3230:
3225:
3220:
3215:
3210:
3205:
3200:
3195:
3190:
3124:
2959:
2790:
2785:
2752:
2747:
2742:
2594:
2589:
2455:
2450:
2445:
2435:
2430:
2425:
2420:
2415:
2410:
2405:
2400:
2395:
2390:
2385:
2380:
2137:
2132:
1978:
1973:
1968:
1963:
1582:
1478:
1448:
728:
579:
575:
560:
555:
Size comparison of supergiant and hypergiant stars, including Cygnus OB2 #12,
521:
468:
407:
374:
323:
236:
3185:
3180:
3175:
3170:
3148:
2709:
2679:
2564:
2375:
2370:
2360:
2355:
2350:
2345:
2340:
2335:
2330:
2325:
2315:
2310:
2305:
2300:
2295:
2290:
2285:
2280:
2275:
2270:
2265:
2260:
2255:
2250:
2245:
2240:
2235:
2230:
2225:
2220:
2215:
2210:
2205:
2200:
2195:
2190:
2185:
2180:
2114:
2109:
2104:
2099:
2094:
2089:
2071:
2066:
2061:
2056:
2008:
1687:
1682:
1677:
1667:
1657:
1652:
1647:
1587:
595:
564:
533:
1320:
1285:
1203:
1168:
1488:
3446:
3165:
3129:
3103:
3098:
3093:
3014:
3009:
3004:
2999:
2994:
2989:
2984:
2954:
2911:
2820:
2815:
2810:
2805:
2800:
2795:
2619:
2175:
2170:
2165:
1958:
1953:
1948:
1943:
1938:
1933:
1928:
1923:
1918:
1875:
1870:
1865:
1860:
1855:
1850:
1845:
1840:
1835:
1830:
1825:
1820:
1815:
1810:
1805:
1800:
1795:
1790:
1785:
1780:
1775:
1770:
1765:
1760:
1755:
1750:
1745:
1642:
1637:
1632:
1627:
1622:
1617:
1002:
449:
590:, the star would have a visual magnitude about 1.5, nearly as bright as
3465:
3451:
3441:
2936:
2931:
2888:
2780:
2699:
2674:
2669:
2629:
2624:
2523:
2160:
2142:
1993:
1913:
1908:
1903:
1898:
1893:
1740:
1735:
1730:
1725:
1707:
1702:
1562:
708:
46:
1019:
3119:
3076:
2861:
2664:
2659:
2548:
2543:
2538:
2533:
2528:
2518:
2513:
2508:
2503:
2498:
1343:
Van
Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".
830:
636:
583:
503:
434:
387:
328:
1286:"Disentangling the spatial substructure of Cygnus OB2 from Gaia DR2"
846:
Caballero-Nieves, S. M.; Nelan, E. P.; Gies, D. R.; Wallace, D. J.;
1402:
1302:
1245:
1185:
1064:
936:
911:
793:
2979:
2893:
2849:
2654:
1557:
1431:
1357:
1128:
864:
707:
614:
591:
550:
476:
3275:
2775:
1540:
292:
280:
229:
1492:
2365:
2320:
1169:"On the nature of high reddening of Cygnus OB2 #12 hypergiant"
689:, and a mass much lower than the currently accepted ~110
777:
Data
Release 3. Summary of the content and survey properties"
574:
Cygnus OB2 #12 is generally assumed to be a member of the
771:
Vallenari, A.; et al. (Gaia collaboration) (2023).
633:
parallax for Cygnus OB2 #12 indicated a distance around
1484:
http://jumk.de/astronomie/big-stars/cygnus-ob2-12.shtml
528:(all electromagnetic radiation) of −10.9, among the
3473:
3464:
3409:
3156:
3147:
3112:
3084:
3075:
3046:
3028:
2945:
2902:
2869:
2860:
2833:
2761:
2733:
2722:
2557:
2489:
2151:
2123:
2080:
2047:
1884:
1716:
1548:
1539:
1290:Monthly Notices of the Royal Astronomical Society
1173:Monthly Notices of the Royal Astronomical Society
696:. This would put the star’s luminosity below the
668:is more precise and indicates a distance around
578:, a cluster of young massive stars about 4,600
1504:
8:
963:CDS/ADC Collection of Electronic Catalogues
114:41° 14′ 29.279″
3470:
3153:
3081:
2866:
2730:
1545:
1511:
1497:
1489:
1226:
1224:
1222:
1041:
1039:
1037:
1430:
1401:
1356:
1319:
1301:
1244:
1202:
1184:
1127:
1081:
1063:
1001:
935:
863:
810:
792:
74:J2000
1109:
1107:
1105:
1103:
1101:
951:
949:
947:
752:
272:
905:
903:
901:
899:
33:
1474:Online Astronomy: The Brightest Stars
766:
764:
762:
760:
758:
756:
19:The correct title of this article is
7:
841:
839:
63:Location of Cygnus OB2 #12 (circled)
609:companion could be detected in the
284:
14:
654:, and a current mass of 25
52:
45:
827:Gaia DR3 record for this source
307:0.5895 ± 0.0518
912:"Catalog of Galactic OB Stars"
723:Cygnus OB2 #12 is a candidate
520:is an extremely luminous blue
1:
682:, a radius of about 100
1116:Astronomy & Astrophysics
543:and the period as 30 years.
1263:10.1051/0004-6361/201935141
1146:10.1051/0004-6361/201117472
812:10.1051/0004-6361/202243940
727:(LBV). Its position in the
3554:
1375:10.1051/0004-6361:20078357
1345:Astronomy and Astrophysics
1233:Astronomy and Astrophysics
882:10.1088/0004-6256/147/2/40
781:Astronomy and Astrophysics
741:List of most massive stars
491: 2067782734461462912
18:
1526:
1449:10.1134/S1063772913070019
1052:The Astrophysical Journal
910:Reed, B. Cameron (2003).
530:most luminous stars known
496:
479: J20324096+4114291,
466:
459:
455:
361:
356:
352:
242:
235:
131:
68:
39:
1083:10.3847/1538-4357/aa7e79
916:The Astronomical Journal
852:The Astronomical Journal
698:Humphreys-Davidson limit
613:. However, analysis of
3523:Luminous blue variables
1531:List of stars in Cygnus
1520:Constellation of Cygnus
1367:2007A&A...474..653V
1255:2019A&A...627A..99N
1138:2012A&A...541A.145C
803:2023A&A...674A...1G
719:image of Cygnus OB2 #12
647:, a radius of 118
338:Absolute magnitude
192:Apparent magnitude
181:Apparent magnitude
170:Apparent magnitude
159:Apparent magnitude
121:Apparent magnitude
3513:Cygnus (constellation)
3135:ZTF J203349.8+322901.1
725:luminous blue variable
720:
571:
29:technical restrictions
23:. The omission of the
711:
621:creating the x-rays.
554:
2917:North America Nebula
1479:Tim Thompson: OB2-12
1321:10.1093/mnras/stz117
1204:10.1093/mnras/stw385
848:Degioia-Eastwood, K.
526:bolometric magnitude
16:Blue hypergiant star
3538:Suspected variables
1441:2013ARep...57..527C
1312:2019MNRAS.484.1838B
1195:2016MNRAS.458..491M
1074:2017ApJ...845...39O
1012:2004ARep...48.1005K
975:2003yCat.2246....0C
928:2003AJ....125.2531R
874:2014AJ....147...40C
666:Gaia Data Release 3
631:Gaia Data Release 2
576:Cyg OB2 Association
497:Database references
36:
3528:B-type hypergiants
3020:Soap Bubble Nebula
721:
572:
461:Other designations
327:(1,700 ± 100
287: −3.412
275: −1.703
225:Variable type
148:Apparent magnitude
138:Spectral type
34:
3518:Hipparcos objects
3500:
3499:
3496:
3495:
3460:
3459:
3143:
3142:
3071:
3070:
3064:
2853:
2829:
2828:
2718:
2717:
1419:Astronomy Reports
1020:10.1134/1.1836024
996:(12): 1005–1018.
990:Astronomy Reports
524:with an absolute
515:
514:
322:5,500 ± 500
3545:
3471:
3154:
3082:
3058:
2867:
2847:
2731:
1546:
1513:
1506:
1499:
1490:
1461:
1460:
1434:
1414:
1408:
1407:
1405:
1393:
1387:
1386:
1360:
1340:
1334:
1333:
1323:
1305:
1281:
1275:
1274:
1248:
1228:
1217:
1216:
1206:
1188:
1164:
1158:
1157:
1131:
1111:
1096:
1095:
1085:
1067:
1043:
1032:
1031:
1005:
1003:astro-ph/0605483
985:
979:
978:
953:
942:
941:
939:
922:(5): 2531–2533.
907:
894:
893:
867:
843:
834:
824:
814:
796:
768:
671:
639:
569:VY Canis Majoris
286:
274:
259:−11.00 km/s
132:Characteristics
124:
104:
99:
69:Observation data
56:
49:
37:
3553:
3552:
3548:
3547:
3546:
3544:
3543:
3542:
3503:
3502:
3501:
3492:
3456:
3405:
3139:
3108:
3067:
3042:
3038:Crescent Nebula
3024:
2970:IRAS 20324+4057
2965:IRAS 19475+3119
2941:
2898:
2856:
2836:
2825:
2757:
2725:
2714:
2705:WISE J2000+3629
2615:GSC 03949-00967
2553:
2485:
2147:
2119:
2076:
2043:
1880:
1712:
1535:
1522:
1517:
1470:
1465:
1464:
1416:
1415:
1411:
1395:
1394:
1390:
1342:
1341:
1337:
1283:
1282:
1278:
1230:
1229:
1220:
1166:
1165:
1161:
1113:
1112:
1099:
1045:
1044:
1035:
987:
986:
982:
955:
954:
945:
909:
908:
897:
845:
844:
837:
770:
769:
754:
749:
737:
706:
695:
692:
688:
685:
681:
678:
669:
660:
657:
653:
650:
646:
643:
634:
627:
619:colliding winds
549:
542:
539:
492:
420:
417:
413:1,660,000
400:
397:
380:
377:
343:
326:
283:
254:
249:Radial velocity
119:
102:
97:Right ascension
95:
70:
64:
62:
61:
60:
59:
58:
57:
35:Cygnus OB2 #12
32:
17:
12:
11:
5:
3551:
3549:
3541:
3540:
3535:
3530:
3525:
3520:
3515:
3505:
3504:
3498:
3497:
3494:
3493:
3491:
3490:
3485:
3479:
3477:
3468:
3462:
3461:
3458:
3457:
3455:
3454:
3449:
3444:
3439:
3434:
3429:
3424:
3419:
3413:
3411:
3407:
3406:
3404:
3403:
3398:
3393:
3388:
3383:
3378:
3373:
3368:
3363:
3358:
3353:
3348:
3343:
3338:
3333:
3328:
3323:
3318:
3313:
3308:
3303:
3298:
3293:
3288:
3283:
3278:
3273:
3268:
3263:
3258:
3253:
3248:
3243:
3238:
3233:
3228:
3223:
3218:
3213:
3208:
3203:
3198:
3193:
3188:
3183:
3178:
3173:
3168:
3162:
3160:
3151:
3145:
3144:
3141:
3140:
3138:
3137:
3132:
3127:
3122:
3116:
3114:
3110:
3109:
3107:
3106:
3101:
3096:
3090:
3088:
3079:
3073:
3072:
3069:
3068:
3066:
3065:
3052:
3050:
3044:
3043:
3041:
3040:
3034:
3032:
3026:
3025:
3023:
3022:
3017:
3012:
3007:
3002:
2997:
2992:
2987:
2982:
2977:
2972:
2967:
2962:
2957:
2951:
2949:
2943:
2942:
2940:
2939:
2934:
2929:
2924:
2922:Pelican Nebula
2919:
2914:
2908:
2906:
2900:
2899:
2897:
2896:
2891:
2886:
2881:
2875:
2873:
2864:
2858:
2857:
2855:
2854:
2841:
2839:
2831:
2830:
2827:
2826:
2824:
2823:
2818:
2813:
2808:
2803:
2798:
2793:
2788:
2783:
2778:
2773:
2767:
2765:
2759:
2758:
2756:
2755:
2750:
2745:
2739:
2737:
2728:
2720:
2719:
2716:
2715:
2713:
2712:
2707:
2702:
2697:
2692:
2687:
2685:PSR J2032+4127
2682:
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2585:Cygnus OB2 #12
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1468:External links
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1425:(7): 527–547.
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489:Gaia DR2
486:
483: 13138,
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266:Proper motion
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111:
108:
107:
103:20 32 40.9572
101:
98:
94:
93:
90:
87:
85:
84:Constellation
82:
81:
77:
73:
67:
55:
48:
38:
30:
26:
22:
2695:W75N(B)-VLA2
2650:KIC 11145123
2645:KIC 11026764
2584:
1422:
1418:
1412:
1391:
1348:
1344:
1338:
1293:
1289:
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1115:
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989:
983:
966:
962:
919:
915:
855:
851:
784:
780:
774:
722:
674:
663:
628:
600:
598:to be seen.
582:(1,400
573:
557:V382 Carinae
517:
516:
502:
469:Cyg OB2
441:
433:13,700
426:
406:
386:
366:
336:
315:
299:
264:
247:
197:2.704±0.364
186:3.512±0.260
175:4.667±0.324
20:
3437:HD 191806 b
3427:HD 187123 b
3422:HD 185269 b
3061:Veil Nebula
3059:(including
3056:Cygnus Loop
2927:Sadr Region
2884:Barnard 147
2879:Barnard 146
2848:(including
2771:Berkeley 86
2735:Association
2690:SPECULOOS-3
2640:KIC 9832227
2635:KIC 8462852
2600:G79.29+0.46
2570:BD+40° 4210
1578:ε (Aljanah)
1573:δ (Fawaris)
1563:β (Albireo)
1296:(2): 1838.
580:light-years
471: #12,
428:Temperature
215:color index
204:color index
110:Declination
3507:Categories
3276:64b (PH1b)
3149:Exoplanets
2960:Egg Nebula
2791:Messier 39
2786:Messier 29
2753:Cygnus OB9
2748:Cygnus OB7
2743:Cygnus OB2
2595:Cygnus X-3
2590:Cygnus X-1
2575:BD+43 3654
1403:2301.08916
1303:1901.02959
1246:1906.00762
1186:1602.05042
1065:1707.04473
969:: II/246.
794:2208.00211
747:References
729:HR diagram
704:Properties
664:The later
588:extinction
561:Betelgeuse
547:Cygnus OB2
522:hypergiant
475: 12,
408:Luminosity
237:Astrometry
194: (K)
183: (H)
172: (J)
161: (V)
150: (B)
27:is due to
3417:b Cygni b
3125:4C +48.48
2947:Planetary
2835:Molecular
2710:Wolf 1069
2680:N6946-BH1
2565:AFGL 2591
1718:Flamsteed
1558:α (Deneb)
1457:123003317
1432:1306.1087
1358:0708.1752
1330:118869784
1271:173990444
1213:118824868
1129:1202.3991
1092:119537489
1058:(1): 39.
865:1311.5087
858:(2): 40.
821:244398875
635:840
596:telescope
565:VV Cephei
448:3.0
393:246
373:110
142:B3–4 Ia+
123: (V)
3466:Exomoons
3447:KELT-20b
3130:Cygnus A
3077:Galaxies
3015:NGC 7048
3010:NGC 7027
3005:NGC 7026
3000:NGC 7008
2995:NGC 6884
2990:NGC 6881
2985:NGC 6826
2955:Abell 78
2912:NGC 6914
2845:Cygnus X
2821:NGC 6910
2816:NGC 6871
2811:NGC 6866
2806:NGC 6834
2801:NGC 6819
2796:NGC 6811
2726:clusters
2620:HAT-P-17
2610:G 208-45
2605:G 208-44
2366:86 (PH2)
2321:64 (PH1)
1886:Variable
1568:γ (Sadr)
1383:18759600
1154:11978733
1122:: A145.
1028:55121658
890:22036552
735:See also
717:infrared
694:☉
687:☉
680:☉
659:☉
652:☉
645:☉
625:Distance
611:spectrum
541:☉
419:☉
399:☉
379:☉
340: (M
317:Distance
301:Parallax
3488:1708b I
3483:1625b I
3452:TrES-5b
3442:KELT-9b
2937:Sh2-106
2932:Sh2-101
2889:IC 5146
2862:Nebulae
2781:IC 5146
2700:WASP-48
2675:MWC 349
2670:KOI-256
2630:KELT-20
1437:Bibcode
1363:Bibcode
1308:Bibcode
1251:Bibcode
1239:: A99.
1191:Bibcode
1134:Bibcode
1070:Bibcode
1008:Bibcode
971:Bibcode
924:Bibcode
870:Bibcode
799:Bibcode
532:in the
473:Schulte
357:Details
127:11.702
76:Equinox
3475:Kepler
3158:Kepler
3120:3C 438
2837:clouds
2665:KOI-81
2660:KOI-74
2625:KELT-9
2153:Kepler
2125:Gliese
2115:197037
2110:191806
2105:188753
2100:187123
2095:185435
2090:185269
1861:71 (g)
1856:68 (A)
1851:63 (f)
1841:59 (f)
1791:29 (b)
1786:28 (b)
1781:27 (b)
1776:26 (e)
1761:20 (d)
1751:16 (c)
1455:
1381:
1328:
1269:
1211:
1152:
1090:
1026:
888:
831:VizieR
819:
787:: A1.
713:UKIDSS
567:, and
534:galaxy
504:SIMBAD
388:Radius
164:11.40
153:14.41
89:Cygnus
78:J2000
3410:Other
3401:1708b
3391:1649b
3386:1658b
3381:1652b
3376:1625b
3371:1520b
3366:1229b
3113:Other
2980:M1-92
2894:L1014
2850:DR 21
2655:KOI-5
2558:Other
2039:V2513
2034:V2214
2029:V1974
2024:V1794
2019:V1668
2014:V1500
2009:V1489
2004:V1334
1999:V1191
1994:V1143
1989:V1057
1984:V1027
1550:Bayer
1541:Stars
1453:S2CID
1427:arXiv
1398:arXiv
1379:S2CID
1353:arXiv
1326:S2CID
1298:arXiv
1267:S2CID
1241:arXiv
1209:S2CID
1181:arXiv
1150:S2CID
1124:arXiv
1088:S2CID
1060:arXiv
1024:S2CID
998:arXiv
886:S2CID
860:arXiv
825:
817:S2CID
789:arXiv
715:near-
615:x-ray
592:Deneb
477:2MASS
348:−9.82
285:Dec.:
219:3.01
208:1.69
72:Epoch
3361:737b
3356:560b
3351:452b
3346:451b
3341:432b
3336:419b
3331:409b
3321:371b
3306:186b
3104:7013
3099:6946
3094:6801
2904:H II
2871:Dark
2776:DR 6
2763:Open
2724:Star
2524:138a
2481:1708
2476:1649
2471:1625
2466:1520
2461:1229
2143:1245
2072:8193
2067:7912
2062:7767
2057:7633
1979:V476
1974:V404
1969:V389
1964:V380
1177:1602
967:2246
775:Gaia
661:.
629:The
510:data
368:Mass
230:cLBV
213:B−V
202:U−B
3301:87c
3296:78b
3291:70b
3286:69b
3281:68b
3271:61b
3266:56b
3261:47b
3256:41b
3251:40b
3246:39b
3241:36b
3236:34b
3231:33b
3226:32b
3221:28b
3216:23b
3211:22b
3206:17b
3201:16b
3196:15b
3191:11b
3086:NGC
3048:SNR
2549:150
2544:148
2539:147
2534:142
2529:140
2519:137
2514:136
2509:135
2504:134
2499:133
2456:737
2451:560
2446:452
2441:451
2436:445
2431:432
2426:419
2421:411
2416:385
2411:371
2406:289
2401:223
2396:186
2391:182
2386:167
2381:107
2138:806
2133:777
1445:doi
1371:doi
1349:474
1316:doi
1294:484
1259:doi
1237:627
1199:doi
1142:doi
1120:541
1078:doi
1056:845
1016:doi
932:doi
920:125
878:doi
856:147
829:at
807:doi
785:674
485:HIP
481:NSV
450:Myr
443:Age
309:mas
303:(π)
289:mas
277:mas
273:RA:
268:(μ)
3509::
3186:6b
3181:5b
3176:3c
3171:3b
3166:2b
3030:WR
2491:WR
2376:89
2371:87
2361:84
2356:80
2351:78
2346:70
2341:69
2336:68
2331:67
2326:66
2316:63
2311:61
2306:56
2301:51
2296:47
2291:45
2286:44
2281:43
2276:42
2271:41
2266:40
2261:39
2256:36
2251:35
2246:34
2241:33
2236:32
2231:31
2226:29
2221:28
2216:27
2211:23
2206:22
2201:18
2196:17
2191:16
2186:15
2181:11
2082:HD
2049:HR
1959:KY
1954:CH
1949:BI
1944:BC
1939:AZ
1934:TT
1929:SU
1924:SS
1919:RW
1876:75
1871:74
1866:72
1846:61
1836:57
1831:56
1826:55
1821:52
1816:47
1811:41
1806:39
1801:35
1796:33
1771:23
1766:22
1756:17
1746:15
1451:.
1443:.
1435:.
1423:57
1421:.
1377:.
1369:.
1361:.
1347:.
1324:.
1314:.
1306:.
1292:.
1288:.
1265:.
1257:.
1249:.
1235:.
1221:^
1207:.
1197:.
1189:.
1175:.
1171:.
1148:.
1140:.
1132:.
1118:.
1100:^
1086:.
1076:.
1068:.
1054:.
1050:.
1036:^
1022:.
1014:.
1006:.
994:48
992:.
965:.
961:.
946:^
930:.
918:.
914:.
898:^
884:.
876:.
868:.
854:.
838:^
815:.
805:.
797:.
783:.
779:.
755:^
700:.
637:pc
584:pc
563:,
559:,
329:pc
324:ly
293:yr
281:yr
251:(R
3432:c
3396:c
3326:c
3316:f
3311:e
3063:)
2852:)
2176:6
2171:5
2166:3
2161:2
1914:Y
1909:X
1904:W
1899:T
1894:R
1741:9
1736:8
1731:4
1726:2
1708:Q
1703:P
1698:ω
1693:ω
1688:ψ
1683:χ
1678:φ
1673:υ
1668:τ
1663:σ
1658:ρ
1653:π
1643:ο
1638:o
1633:o
1628:ξ
1623:ν
1618:μ
1613:λ
1608:κ
1603:ι
1598:ι
1593:θ
1588:η
1583:ζ
1512:e
1505:t
1498:v
1459:.
1447::
1439::
1429::
1406:.
1400::
1385:.
1373::
1365::
1355::
1332:.
1318::
1310::
1300::
1273:.
1261::
1253::
1243::
1215:.
1201::
1193::
1183::
1156:.
1144::
1136::
1126::
1094:.
1080::
1072::
1062::
1030:.
1018::
1010::
1000::
977:.
973::
940:.
934::
926::
892:.
880::
872::
862::
833:.
823:.
809::
801::
791::
773:"
691:M
684:R
677:L
656:M
649:R
642:L
538:M
435:K
416:L
396:R
376:M
344:)
342:V
331:)
291:/
279:/
255:)
253:v
31:.
25:#
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