R136a3: Perbedaan antara revisi
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{{Starbox observe|epoch=J2000|equinox=[[J2000.0]]|ra={{RA|05|38|42.33}}<ref name=census/>|dec={{DEC|−69|06|03.27}}<ref name=census/>|constell=[[Dorado]]|appmag_v=12.97<ref name="census">{{cite journal |title=The VLT-FLAMES Tarantula Survey. XI. A census of the hot luminous stars and their feedback in 30 Doradus |journal=Astronomy & Astrophysics |last1=Doran |first1=E. I. |last2=Crowther |first2=P. A. |last3=De Koter |first3=A. |last4=Evans |first4=C. J. |last5=McEvoy |first5=C. |last6=Walborn |first6=N. R. |last7=Bastian |first7=N. |last8=Bestenlehner |first8=J. M. |last9=Gräfener |first9=G. |last10=Herrero |first10=A. |last11=Köhler |first11=K. |last12=Maíz Apellániz |first12=J. |last13=Najarro |first13=F. |last14=Puls |first14=J. |last15=Sana |first15=H. |last16=Schneider |first16=F. R. N. |last17=Taylor |first17=W. D. |last18=Van Loon |first18=J. Th. |last19=Vink |first19=J. S. |display-authors=5 |volume=558 |at=A134 |date=October 2013 |doi=10.1051/0004-6361/201321824 |bibcode=2013A&A...558A.134D |arxiv=1308.3412}}</ref>}}
{{Starbox character|type=[[Bintang Wolf–Rayet]]|class=[[Bintang Wolf–Rayet|WN5h]]<ref name=crowther2016/>}}
{{Starbox astrometry|dist_ly=163,000|dist_pc=49,970<ref name="Nature">{{cite journal |title=An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent |journal=Nature |last1=Pietrzyński |first1=G. |last2=Graczyk |first2=D. |last3=Gieren |first3=W. |last4=Thompson |first4=I. B. |last5=Pilecki |first5=B. |last6=Udalski |first6=A. |last7=Soszyński |first7=I. |display-authors=5 |volume=495 |issue=7439 |pages=76–79 |date=March 2013 |doi=10.1038/nature11878 |pmid=23467166 |arxiv=1303.2063 |bibcode=2013Natur.495...76P}}</ref>|absmag_v=
{{Starbox detail|source=<ref name="crowther2016">{{cite journal |title=The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters |journal=Monthly Notices of the Royal Astronomical Society |last1=Crowther |first1=Paul A. |last2=Caballero-Nieves |first2=S. M. |last3=Bostroem |first3=K. A. |last4=Maíz Apellániz |first4=J. |last5=Schneider |first5=F. R. N. |last6=Walborn |first6=N. R. |last7=Angus |first7=C. R. |last8=Brott |first8=I. |last9=Bonanos |first9=A. |last10=De Koter |first10=A. |last11=De Mink |first11=S. E. |last12=Evans |first12=C. J. |last13=Gräfener |first13=G. |last14=Herrero |first14=A. |last15=Howarth |first15=I. D. |last16=Langer |first16=N. |last17=Lennon |first17=D. J. |last18=Puls |first18=J. |last19=Sana |first19=H. |last20=Vink |first20=J. S. |display-authors=5 |volume=458 |issue=1 |pages=624–659 |date=May 2016 |doi=10.1093/mnras/stw273 |bibcode=2016MNRAS.458..624C |arxiv=1603.04994}}</ref>|mass=180|luminosity=3,800,000|temperature=53,000|radius=19<ref name="hainich">{{cite journal |title=The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class |journal=Astronomy & Astrophysics |last1=Hainich |first1=R. |last2=Rühling |first2=U. |last3=Todt |first3=H. |last4=Oskinova |first4=L. M. |last5=Liermann |first5=A. |last6=Gräfener |first6=G. |last7=Foellmi |first7=C. |last8=Schnurr |first8=O. |last9=Hamann |first9=W.-R. |display-authors=5 |volume=565 |at=A27 |date=May 2014 |doi=10.1051/0004-6361/201322696 |bibcode=2014A&A...565A..27H |arxiv=1401.5474}}</ref>|age_myr=0.3}}
{{Starbox catalog|names=RMC 136a3, [[BAT99]] 106}}
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