474:. In 2007, together with a few collaborators, he predicted the existence of massive stars with properties very similar to VFTS 102. In its theoretical model, the extreme rotational speed is caused by the transfer of material from a companion star in a binary system. After this "cosmic dance", the donor star is predicted to explode as a supernova. The spun-up companion instead is likely to be launched out of the orbit and move away from its stellar neighbors at high speed. Such a star is called a runaway. VFTS 102 fits this theoretical model very well, being found to be a rapidly rotating runaway star and lying close to a pulsar and a supernova remnant. Other scenarios, like a dynamical ejection from the core of the star cluster R136, are also possible.
28:
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397:
455:. The resulting centripetal force tends to flatten the star; material can be lost in the loosely bound equatorial regions, allowing for the formation of a disk. The spectroscopic observations seem to confirm this, and the star is classified as Oe, possibly due to emission from such an equatorial disk of gas.
498:
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
535:
Bonanos, A. Z.; Massa, D. L.; Sewilo, M.; Lennon, D. J.; Panagia, N.; Smith, L. J.; Meixner, M.; Babler, B. L.; Bracker, S.; Meade, M. R.; Gordon, K. D.; Hora, J. L.; Indebetouw, R.; Whitney, B. A. (2009). "Spitzer SAGE Infrared
Photometry of Massive Stars in the Large Magellanic Cloud".
598:; Fraser, M.; Hénault-Brunet, V.; Howarth, I. D.; Langer, N.; Lennon, D. J.; Markova, N.; Sana, H.; Taylor, W. D. (2011). "The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?".
908:
499:
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).
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Cantiello, M.; Yoon, S.-C.; Langer, N.; Livio, M. (2007). "Binary star progenitors of long gamma-ray bursts".
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774:"The Galactic WC stars. Stellar parameters from spectral analyses indicate a new evolutionary sequence"
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466:, an Italian astrophysicist who emigrated to the United States and is currently working at the
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715:"The binary merger channel for the progenitor of the fastest rotating O-type star VFTS 102"
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This star was observed by the VLT Flames
Tarantula Survey collaboration using the VLT,
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Dufton, P. L.; Dunstall, P. R.; Evans, C. J.; Brott, I.; Cantiello, M.; De Koter, A.;
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436:), making it the second fastest rotating massive star known alongside
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The peculiarity of this star is its projected equatorial velocity of ~
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Jiang, Dengkai; Han, Zhanwen; Yang, Liheng; Li, Lifang (2013).
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Press
Release at University of California Santa Barbara
656:"HST/COS Spectra of the Wind Lines of VFTS 102 and 285"
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772:Sander, A.; Hamann, W.-R.; Todt, H. (April 2012).
719:Monthly Notices of the Royal Astronomical Society
83:−69° 09′ 51.04″
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8:
400:The position of VFTS 102 in Tarantula nebula
505:CDS/ADC Collection of Electronic Catalogues
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18:
919:VLT Flames Tarantuala Survey Homepage
462:in Chile. One member of this team is
7:
444:), and preceded only by the WO star
2132:Stars in the Large Magellanic Cloud
654:Shepard, Katherine (January 2020).
448:which has a rotational velocity of
198:
14:
600:The Astrophysical Journal Letters
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411:, a star forming region in the
26:
16:Star in the constellation Dorado
32:Artistic depiction of VFTS 102
1:
904:News on "Corriere della Sera"
568:10.1088/0004-6256/138/4/1003
415:, a satellite galaxy of the
976:Dorado in Chinese astronomy
808:10.1051/0004-6361/201117830
630:10.1088/2041-8205/743/1/L22
2163:
2112:O-type main-sequence stars
869:10.1051/0004-6361:20077115
839:Astronomy and Astrophysics
778:Astronomy and Astrophysics
2085:
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924:Matteo Cantiello HomePage
660:The Astrophysical Journal
407:is a star located in the
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691:10.3847/1538-4357/ab5a82
538:The Astronomical Journal
370: J05373924-6909510
971:List of stars in Dorado
960:Constellation of Dorado
861:2007A&A...465L..29C
800:2012A&A...540A.144S
107:Evolutionary stage
90:Apparent magnitude
1997:Large Magellanic Cloud
413:Large Magellanic Cloud
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1917:Tarantula Nebula (30)
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909:News on "Il Tirreno"
750:10.1093/mnras/sts105
460:Very Large Telescope
2137:Extragalactic stars
2117:Emission-line stars
2060:Astronomical events
899:STScI Press Release
741:2013MNRAS.428.1218J
682:2020ApJ...888...82S
622:2011ApJ...743L..22D
560:2009AJ....138.1003B
517:2003yCat.2246....0C
376:Database references
336:Rotational velocity
21:
1288:MACHO 80.7443.1718
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360:Other designations
119:Spectral type
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981:Sanduleak -69 202
894:ESO Press Release
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350:610±30 km/s
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1093:
1091:
1089:
1085:
1079:
1076:
1074:
1071:
1069:
1066:
1064:
1061:
1059:
1056:
1054:
1051:
1049:
1046:
1044:
1041:
1039:
1036:
1034:
1031:
1029:
1026:
1024:
1021:
1019:
1016:
1014:
1011:
1009:
1006:
1005:
1003:
1001:
997:
994:
992:
988:
982:
979:
977:
974:
972:
969:
968:
965:
961:
954:
949:
947:
942:
940:
935:
934:
931:
925:
922:
920:
917:
915:
912:
910:
907:
905:
902:
900:
897:
895:
892:
891:
887:
878:
874:
870:
866:
862:
858:
853:
848:
844:
840:
833:
830:
825:
821:
817:
813:
809:
805:
801:
797:
792:
787:
783:
779:
775:
768:
765:
760:
756:
751:
746:
742:
738:
733:
728:
724:
720:
716:
709:
706:
701:
697:
692:
687:
683:
679:
674:
669:
665:
661:
657:
650:
648:
644:
639:
635:
631:
627:
623:
619:
614:
609:
605:
601:
597:
590:
588:
586:
582:
577:
573:
569:
565:
561:
557:
552:
547:
543:
539:
531:
529:
527:
523:
518:
514:
510:
506:
502:
494:
492:
490:
488:
484:
477:
475:
473:
469:
465:
461:
456:
453:
447:
442:609 km/s
439:
434:
427:
420:
418:
414:
410:
406:
398:
390:
387:
385:
384:
380:
379:
374:
369:
364:
361:
357:
353:
349:
347:
345:
341:
337:
333:
332:
329:
324:36,000 ± 5000
322:
320:
319:
315:
314:
311:
304:
302:
300:
296:
292:
291:
288:
276:
274:
273:
269:
268:
265:
253:
251:
250:
246:
245:
241:
236:
232:
228:
225:(50,000
223:
220:164,000
219:
217:
216:
212:
211:
208:
204:
196:
192:
185:
183:
181:
180:Proper motion
177:
176:
173:228 km/s
172:
170:
164:
160:
159:
155:
152:
148:
144:
142:
138:
137:
134:−0.879
133:
131:
127:
126:
122:
120:
117:
116:
113:
112:Main sequence
110:
108:
105:
104:
99:
95:
91:
87:
86:
82:
80:
77:
76:
70:
67:
63:
62:
59:
56:
54:
53:Constellation
51:
50:
46:
42:
36:
29:
23:
2037:Dorado Group
1443:Gliese 163 c
1391:
1268:LHA 120-S 79
1253:HE 0437-5439
842:
838:
832:
781:
777:
767:
722:
718:
708:
663:
659:
603:
599:
541:
537:
508:
504:
457:
421:
404:
403:
381:
343:
339:
334:
316:
298:
293:
270:
247:
213:
178:
161:
72:05 37 39.248
2068:GRB 790305b
1999:(partly in
1377:SGR 0525−66
725:(2): 1218.
318:Temperature
141:color index
130:color index
79:Declination
2106:Categories
2011:LEDA 89996
1473:TOI-4127 b
1453:HD 30177 b
1448:HD 28254 b
1435:Exoplanets
1298:Melnick 42
1293:Melnick 34
1273:LH 41-1042
1248:Gliese 163
845:(2): L29.
673:1911.09675
606:(1): L22.
511:: II/246.
478:References
450:1000
297:(log
272:Luminosity
151:Astrometry
1872:Henize 70
1782:Hodge 301
1571:1854/1855
1468:TOI-813 b
1458:TOI-700 d
1278:LH 54-425
1238:BAT99-123
1233:BAT99-104
877:118921504
824:119182468
816:0004-6361
791:1201.6354
759:118856665
732:1302.6296
700:208202016
666:(2): 82.
638:118448435
613:1111.0157
551:0905.1328
424:610
417:Milky Way
306:3.6 ± 0.5
123:O9:Vnnne
92: (V)
20:VFTS 102
2093:Category
2073:SN 1987A
1931:Galaxies
1489:clusters
1407:VFTS 682
1402:VFTS 352
1397:VFTS 243
1392:VFTS 102
1283:LMC195-1
1228:BAT99-98
1223:BAT99-68
1218:BAT99-66
1088:Variable
784:: A144.
576:14056495
438:VFTS 285
405:VFTS 102
286:☉
263:☉
215:Distance
1801:Nebulae
1417:WOH G64
1387:TOI-813
1382:TOI-700
1213:BAT99-7
857:Bibcode
796:Bibcode
737:Bibcode
678:Bibcode
618:Bibcode
556:Bibcode
513:Bibcode
429:(about
278:100,000
238:Details
145:+0.293
96:15.806
45:Equinox
2142:Dorado
2005:Hydrus
1258:HV 888
1243:BI 253
1192:269810
875:
822:
814:
757:
698:
636:
574:
446:WR 142
383:SIMBAD
326:
308:
280:
257:
58:Dorado
47:J2000
2001:Mensa
1990:Other
1865:Other
1787:LH 95
1775:Other
1201:Other
1187:38282
1182:37974
1177:37836
1172:33579
1167:30177
1162:28254
1157:27274
1096:R (P)
1000:Bayer
991:Stars
873:S2CID
847:arXiv
820:S2CID
786:arXiv
755:S2CID
727:arXiv
696:S2CID
668:arXiv
634:S2CID
608:arXiv
572:S2CID
546:arXiv
368:2MASS
199:Dec.:
41:Epoch
2003:and
1981:2082
1976:1947
1971:1892
1966:1672
1961:1566
1956:1553
1951:1549
1946:1533
1882:N119
1856:2080
1851:2078
1846:2060
1841:2032
1836:2029
1831:2020
1826:2014
1821:1936
1816:1934
1766:2257
1761:2241
1756:2197
1751:2164
1746:2108
1741:2100
1736:2074
1731:2070
1726:2040
1721:2027
1716:2004
1711:2003
1706:2002
1701:2001
1696:1997
1691:1994
1686:1984
1681:1983
1676:1978
1671:1974
1666:1971
1661:1969
1656:1955
1651:1935
1646:1929
1641:1910
1636:1903
1631:1901
1626:1898
1621:1873
1616:1872
1611:1871
1606:1869
1601:1868
1596:1866
1591:1860
1586:1859
1581:1858
1576:1856
1566:1852
1561:1850
1556:1847
1551:1846
1546:1820
1541:1818
1536:1806
1531:1783
1526:1763
1521:1761
1516:1755
1511:1712
1506:1712
1487:Star
1372:R145
1367:R139
1328:R136
1139:2102
1134:1859
812:ISSN
509:2246
452:km/s
433:km/h
426:km/s
389:data
255:~ 25
249:Mass
139:B−V
128:U−B
1939:NGC
1907:N55
1902:N49
1897:N44
1892:N41
1887:N11
1809:NGC
1498:NGC
1323:R99
1318:R85
1208:B90
865:doi
843:465
804:doi
782:540
745:doi
723:428
686:doi
664:888
626:doi
604:743
564:doi
542:138
470:at
310:cgs
203:mas
191:mas
187:RA:
182:(μ)
2108::
1348:a3
1343:a2
1338:a1
1149:HD
1126:HR
1116:BB
1111:AB
1106:WZ
871:.
863:.
855:.
841:.
818:.
810:.
802:.
794:.
780:.
776:.
753:.
743:.
735:.
721:.
717:.
694:.
684:.
676:.
662:.
658:.
646:^
632:.
624:.
616:.
602:.
584:^
570:.
562:.
554:.
540:.
525:^
507:.
503:.
486:^
419:.
227:pc
222:ly
207:yr
195:yr
165:(R
2007:)
1463:e
1360:c
1355:b
1333:a
1101:S
1078:G
1073:π
1068:π
1063:ν
1058:λ
1053:κ
1048:θ
1043:η
1038:η
1033:ζ
1028:ε
1023:δ
1018:γ
1013:β
1008:α
952:e
945:t
938:v
879:.
867::
859::
849::
826:.
806::
798::
788::
761:.
747::
739::
729::
702:.
688::
680::
670::
640:.
628::
620::
610::
578:.
566::
558::
548::
519:.
515::
440:(
346:)
344:i
340:v
338:(
328:K
301:)
299:g
283:L
260:M
229:)
205:/
193:/
169:)
167:v
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