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{{Starbox begin
| name = R136c
}}
{{Starbox image
| image = [[File:ESO - Eso1030a (by).jpg|300px]]
| caption = The bright star to the left of the cluster core is R136c.
}}
{{Starbox observe
| epoch = [[J2000.0]]
| equinox = [[J2000.0]]
| constell = [[劍魚座]]
| ra = {{RA|5|38|42.90}}<ref name=census/>
| dec = {{DEC|−69|06|04.83}}<ref name=census/>
| appmag_v = 12.86<ref name=census/>
}}
{{Starbox character
| type = [[沃爾夫-拉葉星]]
| class = [[沃爾夫-拉葉星|WN5h]]<ref name=crowther2016>{{cite journal|bibcode=2016MNRAS.458..624C|arxiv=1603.04994|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|volume=458|issue=1|pages=624–659|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.|author11-link= Selma de Mink |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.|year=2016|doi=10.1093/mnras/stw273|doi-access=free }}</ref>
}}
{{Starbox astrometry
| radial_v = 
| prop_mo_ra = 
| prop_mo_dec = 
| parallax = 
| p_error = 
| parallax_footnote = 
| dist_ly = 163,000
| dist_pc = 49,970<ref name=Nature>{{cite journal|last=Pietrzyński|first=G|author2=D. Graczyk |author3=W. Gieren |author4=I. B. Thompson |author5=B. Pilecki |author6=A. Udalski |author7=I. Soszyński |display-authors=etal |title=An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent|url=https://archive.org/details/sim_nature-uk_2013-03-07_495_7439/page/76|journal=Nature|date=7 March 2013|volume=495|issue=7439|pages=76–79|doi=10.1038/nature11878|pmid=23467166|arxiv = 1303.2063 |bibcode = 2013Natur.495...76P |s2cid=4417699}}</ref>
| absmag_v = −7.9<ref name=census>{{Cite journal|arxiv=1308.3412v1 |last1= Doran |first1= E. I. |title= The VLT-FLAMES Tarantula Survey - XI. A census of the hot luminous stars and their feedback in 30 Doradus |journal= Astronomy & Astrophysics |volume= 558 |pages= A134 |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= Grafener |first9= G. |last10= Herrero |first10= A. |last11= Kohler |first11= K. |last12= Maiz Apellaniz |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. |date= 2013 |doi= 10.1051/0004-6361/201321824 |bibcode = 2013A&A...558A.134D |s2cid= 118510909 }}</ref>
| space_v_u = 
| space_v_v = 
| space_v_w = 
}}
{{Starbox orbit
| reference = <ref name=shenar2023>{{cite journal |bibcode=2023A&A...679A..36S |title=Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and C |last1=Shenar |first1=T. |last2=Sana |first2=H. |last3=Crowther |first3=P. A. |last4=Bostroem |first4=K. A. |last5=Mahy |first5=L. |last6=Najarro |first6=F. |last7=Oskinova |first7=L. |last8=Sander |first8=A. A. C. |journal=Astronomy and Astrophysics |date=2023 |volume=679 |pages=A36 |doi=10.1051/0004-6361/202346930 |arxiv=2309.13113 }}</ref>
| period_unitless = 17.2051日
| eccentricity = {{val|0.31|0.08}}
| k1 = {{val|51|9}}
}}
{{Starbox detail
| source = <ref name=schneider2018>{{cite journal |title=An excess of massive stars in the local 30 Doradus starburst |year=2018 |bibcode=2018Sci...359...69S |arxiv=1801.03107 |doi=10.1126/science.aan0106 |journal=Science |volume=359 |issue=6371 |pages=69–71 |last1=Schneider |first1= F. R. N. |last2=Sana |first2=H. |last3=Evans |first3=C. J. |last4=Bestenlehner |first4=J. M. |last5=Castro |first5=N. |last6=Fossati |first6=L. |last7=Gräfener |first7=G. |last8=Langer |first8=N. |last9=Ramírez-Agudelo |first9=O. H. |last10=Sabín-Sanjulián |first10=C. |last11=Simón-Díaz |first11=S. |last12=Tramper |first12=F. |last13=Crowther |first13=P. A. |last14=de Koter |first14=A. |last15=de Mink |first15=S. E. |last16=Dufton |first16=P. L. |last17=Garcia |first17=M. |last18=Gieles |first18=M. |last19=Hénault-Brunet |first19=V. |last20=Herrero |first20=A. |last21=Izzard |first21= R. G. |last22=Kalari |first22= V. |last23=Lennon |first23= D. J. |last24=Maíz Apellániz |first24= J. |last25=Markova |first25= N. |last26=Najarro |first26= F. |last27=Podsiadlowski |first27= Ph. |last28=Puls |first28= J. |last29=Taylor |first29= W. D. |last30=van Loon |first30= J. Th. |last31=Vink |first31= J. S. |last32=Norman |first32= C. |pmid=29302009 |s2cid=206658504 }}</ref>
| mass = 142
| luminosity = 3,800,000
| radius = 40.7
| temperature = 42,170
| rotational_velocity = <200
| age_myr = 1.8
}}
{{Starbox catalog
| names= [[BAT99]] 112, RMC 136c, VFTS 1025<ref name=schneider2018/>
}}
{{Starbox reference
| Simbad = RMC+136c
| ARICNS = 
}}
{{Starbox end}}

'''R136c'''可能[[雙星]]系統，位於[[劍魚座]][[R136]]中。R136是[[大麥哲倫雲]][[蜘蛛星雲]][[NGC 2070]]中心的一個緊密的恆星團。

NGC 2070是一個[[疏散星團]]，質量為450,000個太陽質量，包含10,000顆[[恆星]]<ref>{{cite journal | last=Bosch | first=Guillermo |author2=Terlevich, Elena|author2-link=Elena Terlevich |author3=Terlevich, Roberto | title=Gemini/GMOS Search for Massive Binaries in the Ionizing Cluster of 30 Dor | journal=Astronomical Journal | volume=137 |issue=2 | pages=3437–3441 | date=2009 | bibcode=2009AJ....137.3437B | doi=10.1088/0004-6256/137/2/3437|arxiv = 0811.4748 | s2cid=17976455 }}</ref>。R136c的質量為{{Solar mass|142|link=y}}，光度為380萬{{Solar luminosity|link=y}}，是已知質量最大、最亮的恆星之一，同時也是溫度最高的恆星之一，溫度超過40,000K。

R136c於1980年首次被 Feitzinger 解析並命名，同時解析的還有[[R136a]]和[[R136b]]<ref name=Feitzinger>{{cite journal|bibcode=1980A&A....84...50F|title=The central object R 136 in the gas nebula 30 Doradus - Structure, color, mass and excitation parameter|journal=Astronomy and Astrophysics|volume=84|issue=1–2|pages=50|last1=Feitzinger|first1=J. V.|last2=Schlosser|first2=W.|last3=Schmidt-Kaler|first3=T.|last4=Winkler|first4=C.|year=1980}}</ref>。

==參考資料==
{{Reflist}}

[[Category:劍魚座]]
[[Category:沃爾夫-拉葉星]]

R136c - 版本历史

imported>InternetArchiveBot：​Add 1 book for verifiability (20251017sim)) #IABot (v2.0.9.5) (GreenC bot

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