293:
1993:
216:
332:
327:
obtained similar results by comparing images of the shell taken in 1993 and 2018. They found that by 2018 the slightly elliptical shell had major and minor axis of 16.8×15.2 arc seconds, and it was expanding at a rate of 0.152×0.139 arc seconds per year, implying a physical expansion rate of
259:
satellite tracking group at the Tokyo
Observatory, showed that the star had begun its nova event as early as 18:36 UT on 26 January 1963, when it had an magnitude of 8. It had attained its peak brightness, magnitude 3, by 17:38 UT on 30 January 1968.
267:. In the case of V533 Herculis, the pair's orbital period is 3.43 hours. Thorstensen and Taylor analysed spectra of the star in its quiescent state, and concluded that it is a non-eclipsing
934:
2030:
430:
954:
927:
907:
247:
The nova was discovered by the
Swedish amateur astronomer Elis Dahlgren on 6 February 1963, and independently by an American amateur,
28:
2020:
1996:
920:
847:"Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells - I. FH Ser, V533 Her, BT Mon, DK Lac and V476 Cyg"
702:
McQuillin, Rachael; Evans, A.; Wilson, D.; Maxted, P.F.L.; Pollacco, D.; West, R.G.; Hounsell, R.A.; Bode, M.F. (January 2011).
60:
296:
Two images of the shell surrounding V533 Hercules taken 25 years apart, showing the nebula's expansion. Both were taken with
959:
1968:
358:
Santamaria, E.; Guerrero, M.A.; Ramos-Larios, G.; Toala, J.A.; Sabin, L.; Rubio, G.; Quino-Mendoza, J.A. (March 2020).
323:) with a diameter of 10±1.4 arc seconds, surrounding the star. The shell is expanding at 850±150 km/sec. Santamaria
1501:
1496:
304:
1246:
964:
182:
2025:
1826:
1821:
943:
308:
241:
73:
1864:
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1347:
316:
1657:
1319:
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536:
477:
381:
129:
1950:
300:
33:
1309:
886:
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827:
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657:
526:
495:
467:
399:
371:
252:
105:
747:"Spectroscopy and orbital periods of the old novae V533 Herculis, V446 Herculis and X Serpentis"
983:
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56:
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1940:
1411:
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389:
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1481:
1471:
1041:
81:
1889:
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813:
762:
688:
643:
540:
481:
385:
32:
RGB composite color image of the faint shell surrounding V533 Herculis, made from three
2015:
1922:
1111:
1076:
1036:
1026:
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1001:
991:
559:
514:
292:
256:
248:
174:
549:
2009:
1884:
1532:
1527:
1304:
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1106:
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1031:
1016:
996:
890:
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822:
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661:
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583:
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403:
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162:
68:
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831:
320:
283:
1894:
1552:
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1235:
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1189:
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1174:
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1164:
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1144:
1134:
1129:
1066:
1056:
1051:
1046:
264:
222:
219:
215:
94:
626:
Haddock, F.T.; Howard, W.E. III; Malville, J.M.; Selling, T.V. (October 1963).
394:
359:
1935:
1930:
1869:
1603:
1593:
1588:
1441:
1436:
1431:
1426:
1254:
1139:
331:
276:
117:
515:"Far Ultraviolet Spectroscopy of Old Novae. II. RR Pic, V533 Her, and DI Lac"
1904:
1849:
1836:
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1557:
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1519:
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1327:
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490:
455:
272:
568:
27:
1976:
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1700:
1695:
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1670:
1665:
1634:
1629:
1598:
1491:
1476:
1461:
1456:
1451:
863:
804:
263:
All novae are binary stars, with a "donor" star transferring matter to a
1879:
1874:
1859:
1854:
1841:
1486:
1446:
1337:
297:
41:
730:
1831:
1648:
1621:
1421:
1299:
425:
201:
146:
628:"An Upper Limit to the 8000 Mc/S Flux Density of Nova Herculis 1963"
652:
627:
531:
472:
376:
255:
star. Subsequent examination of pre-discovery images, taken by the
330:
291:
214:
186:
974:
233:
167:
37:
916:
675:
Mayall, Margaret W. (December 1963). "Variable Star Notes".
236:
visible to the naked eye, which occurred in 1963 in the
745:
Thorstensen, John R.; Taylor, Cynthia J. (March 2000).
632:
251:, on 7 February 1963. Both reported it to be a 4th
1967:
1921:
1814:
1656:
1647:
1620:
1579:
1518:
1404:
1346:
1318:
1245:
1120:
982:
973:
677:
851:Monthly Notices of the Royal Astronomical Society
792:Monthly Notices of the Royal Astronomical Society
751:Monthly Notices of the Royal Astronomical Society
708:Monthly Notices of the Royal Astronomical Society
460:Monthly Notices of the Royal Astronomical Society
44:at 6563 Å and red = at 6583 Å. From Santamaria
335:The location of V533 Herculis (circled in red)
928:
431:Centre de données astronomiques de Strasbourg
8:
319:show a faint, approximately circular shell (
99:+41° 51′ 22.07″
59:J2000.0
1964:
1918:
1653:
1617:
1576:
1515:
979:
935:
921:
913:
788:"The donor stars of cataclysmic variables"
225:of V533 Herculis, plotted using AAVSO data
880:
862:
821:
803:
770:
729:
719:
651:
607:
558:
548:
530:
489:
471:
393:
375:
456:"The distances to Novae as seen by Gaia"
415:
413:
2031:Objects with variable star designations
345:
315:Images of V533 Herculis taken with the
845:Gill, C.D.; O'Brien, T.J. (May 2000).
621:
619:
454:Schaefer, Bradley E. (December 2018).
449:
447:
353:
351:
349:
18:
786:Knigge, Christian (31 October 2006).
513:Sion, Edward M.; et al. (2017).
7:
271:, implying that the donor star is a
955:Hercules–Corona Borealis Great Wall
704:"Novae in the SuperWASP data base"
360:"Angular Expansion of Nova Shells"
16:Nova in the constellation Hercules
14:
275:. Knigge derived a mass of 0.225
1992:
1991:
882:10.1046/j.1365-8711.2000.03342.x
823:10.1111/j.1365-2966.2006.11096.x
772:10.1046/j.1365-8711.2000.03230.x
721:10.1111/j.1365-2966.2011.19695.x
609:10.1111/j.1468-4004.2006.47129.x
584:"Where have all the novae gone?"
26:
1:
960:Hercules in Chinese astronomy
582:Warner, B. (February 2006).
550:10.3847/1538-3881/153/3/109
2047:
588:Astronomy & Geophysics
305:William Herschel Telescope
1989:
1963:
1917:
1616:
1575:
1514:
965:List of stars in Hercules
950:
944:Constellation of Hercules
364:The Astrophysical Journal
194:
180:
173:
156:
152:
123:
116:
53:
24:
2021:Hercules (constellation)
519:The Astronomical Journal
395:10.3847/1538-4357/ab76c5
309:Nordic Optical Telescope
282:, and a radius of 0.333
1827:2MASX J17201001+2637317
1822:2MASX J16270254+4328340
1543:HD 149026 b (Smertrios)
908:Report (not in English)
600:2006A&G....47a..29W
106:Apparent magnitude
1946:Hercules Superclusters
1845:(NGC 6050 and IC 1179)
336:
317:Hubble Space Telescope
312:
289:, for the donor star.
269:SW Sextantis variable
226:
491:10.1093/mnras/sty2388
334:
307:, and right with the
295:
218:
185:Her, Nova Her 1963,
1969:Astronomical events
873:2000MNRAS.314..175G
814:2006MNRAS.373..484K
763:2000MNRAS.312..629T
689:1963JRASC..57..279M
644:1963PASP...75..456H
541:2017AJ....153..109S
482:2018MNRAS.481.3033S
386:2020ApJ...892...60S
195:Database references
36:images: Blue = 4800
21:
337:
313:
227:
175:Other designations
163:Variable type
19:
2003:
2002:
1985:
1984:
1959:
1958:
1913:
1912:
1846:
1643:
1642:
1612:
1611:
1571:
1570:
1538:HAT-P-14b (Sissi)
1510:
1509:
213:
212:
2038:
1995:
1994:
1965:
1951:Zwicky's Triplet
1941:Hercules Cluster
1919:
1844:
1654:
1618:
1577:
1516:
1482:TrES-3 (Pipoltr)
1452:HAT-P-14 (Franz)
980:
937:
930:
923:
914:
895:
894:
884:
866:
864:astro-ph/0001092
842:
836:
835:
825:
807:
805:astro-ph/0609671
783:
777:
776:
774:
742:
736:
735:
733:
723:
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693:
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672:
666:
665:
655:
623:
614:
613:
611:
579:
573:
572:
562:
552:
534:
510:
504:
503:
493:
475:
466:(3): 3033–3051.
451:
442:
441:
439:
437:
417:
408:
407:
397:
379:
355:
328:850×770 km/sec.
157:Characteristics
144:
143:
142:
109:
89:
84:
54:Observation data
30:
22:
2046:
2045:
2041:
2040:
2039:
2037:
2036:
2035:
2026:1963 in science
2006:
2005:
2004:
1999:
1981:
1955:
1923:Galaxy clusters
1909:
1810:
1639:
1608:
1567:
1506:
1472:GSC 02620-00648
1400:
1342:
1314:
1241:
1116:
997:β (Kornephoros)
969:
946:
941:
904:
899:
898:
844:
843:
839:
785:
784:
780:
744:
743:
739:
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673:
669:
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581:
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512:
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445:
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411:
357:
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135:
104:
87:
82:Right ascension
80:
55:
49:
31:
17:
12:
11:
5:
2044:
2042:
2034:
2033:
2028:
2023:
2018:
2008:
2007:
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1990:
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1961:
1960:
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1953:
1948:
1943:
1938:
1933:
1927:
1925:
1915:
1914:
1911:
1910:
1908:
1907:
1902:
1900:QSR J1819+3845
1897:
1892:
1887:
1882:
1877:
1872:
1867:
1865:Hercules Dwarf
1862:
1857:
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1522:
1512:
1511:
1508:
1507:
1505:
1504:
1502:WISE 1741+2553
1499:
1497:WISE 1738+2732
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1401:
1399:
1398:
1393:
1388:
1383:
1378:
1373:
1368:
1363:
1361:147506 (Hunor)
1358:
1356:146389 (Irena)
1352:
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1344:
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994:
992:α (Rasalgethi)
988:
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968:
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902:External links
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896:
857:(1): 175–182.
837:
798:(2): 484–502.
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757:(3): 629–637.
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714:(1): 330–335.
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653:10.1086/128005
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303:, left at the
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249:Leslie Peltier
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20:V533 Herculis
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1890:MCG+07-33-027
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1885:Markarian 501
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1528:14 Herculis b
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1379:
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1374:
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1369:
1367:
1366:149026 (Ogma)
1364:
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1467:Hercules X-1
1417:Furuhjelm 46
1412:BD +17° 3248
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88:18 14 20.485
45:
1895:PGC 2046648
1548:HD 164922 b
265:white dwarf
223:light curve
220:Visual band
112:3.0 - 15.0
95:Declination
34:narrow band
2010:Categories
1936:Abell 2199
1931:Abell 2152
1870:Hercules A
1604:Palomar 14
1594:Messier 92
1589:Messier 13
1520:Exoplanets
1442:Gliese 686
1437:Gliese 649
1432:Gliese 638
1427:Gliese 623
1042:λ (Maasym)
1037:κ (Marsic)
731:2381/11586
532:1701.05218
525:(3). 109.
473:1809.00180
436:2 December
421:"V533 Her"
377:2002.06749
340:References
257:Baker-Nunn
118:Astrometry
40:, green =
1905:UGC 11105
1850:AT2018cow
1837:A2261-BCG
1563:WASP-103b
1558:TOI-561 b
1122:Flamsteed
1112:ω (Cujam)
1007:δ (Sarin)
891:119433788
662:120169907
500:118925493
404:211132830
370:(1): 60.
273:red dwarf
253:magnitude
108: (V)
1997:Category
1977:LBG-2377
1649:Galaxies
1635:NGC 6210
1630:Abell 39
1599:NGC 6229
1492:WASP-103
1477:Ross 640
1462:HAT-P-67
1457:HAT-P-18
1247:Variable
569:29456254
242:Hercules
189:1811+41
130:Distance
63:J2000.0
1880:IC 4617
1875:IC 1192
1860:IC 1189
1855:IC 1182
1842:Arp 272
1622:Nebulae
1487:TOI-561
1447:GJ 3991
1205:104 (A)
869:Bibcode
832:2616606
810:Bibcode
759:Bibcode
685:Bibcode
683:: 279.
640:Bibcode
596:Bibcode
560:5810142
537:Bibcode
478:Bibcode
382:Bibcode
301:filters
74:Hecules
61:Equinox
1832:3C 345
1422:GD 362
1396:164922
1391:164595
1386:156668
1381:155358
1376:154345
1371:152843
1236:32 Oph
1195:99 (b)
1175:72 (w)
1170:69 (e)
1165:68 (u)
1150:45 (l)
1140:30 (g)
1135:29 (h)
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498:
426:SIMBAD
402:
325:et al.
321:nebula
232:was a
202:SIMBAD
145:
46:et al.
2016:Novae
1815:Other
1405:Other
1310:V1674
984:Bayer
975:Stars
887:S2CID
859:arXiv
828:S2CID
800:arXiv
658:S2CID
527:arXiv
496:S2CID
468:arXiv
400:S2CID
372:arXiv
187:AAVSO
57:Epoch
1806:6560
1801:6452
1796:6308
1791:6263
1786:6261
1781:6239
1776:6212
1771:6207
1766:6181
1761:6166
1756:6158
1751:6078
1746:6061
1741:6057
1736:6056
1731:6055
1726:6054
1721:6053
1716:6052
1711:6047
1706:6046
1701:6045
1696:6044
1691:6043
1686:6042
1681:6041
1676:6040
1671:6039
1666:6028
1338:6806
1333:6697
1328:6669
1305:V838
1300:V777
1295:V772
1290:V533
1285:V446
565:PMID
438:2020
234:nova
208:data
183:V533
136:1202
48:2020
1658:NGC
1230:112
1225:111
1220:110
1215:109
1210:106
1200:102
877:doi
855:314
818:doi
796:373
767:doi
755:312
726:hdl
716:doi
712:419
648:doi
604:doi
555:PMC
545:doi
523:153
486:doi
464:481
390:doi
368:892
244:.
240:of
141:−41
139:+52
2012::
1348:HD
1320:HR
1280:DQ
1275:DI
1270:BL
1265:AM
1260:AC
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298:Hα
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1255:X
1107:ψ
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1097:χ
1092:φ
1087:υ
1082:τ
1077:σ
1072:ρ
1067:π
1062:ο
1057:ξ
1052:ν
1047:μ
1032:ι
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284:R
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277:M
38:Å
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