WOH G64: Perbedaan antara revisi

| radius={{val|1,540|77|fmt=commas}}<ref name=levesque/> - 1,730<ref name=ohnaka/>

| luminosity={{val|282,000|40,000|30,000|fmt=commas}}<ref name=levesque/><ref name=ohnaka>{{Cite journal | last1 = Ohnaka | first1 = K. | last2 = Driebe | first2 = T. | last3 = Hofmann | first3 = K. H. | last4 = Weigelt | first4 = G. | last5 = Wittkowski | first5 = M. | title = Resolving the dusty torus and the mystery surrounding LMC red supergiant WOH G64 | doi = 10.1017/S1743921308028858 | journal = Proceedings of the International Astronomical Union | volume = 4 | pages = 454–458 | year = 2009 | pmid = | pmc = | bibcode = 2009IAUS..256..454O | doi-access = free }}</ref> {{nowrap|(340,000 – 454,000)<ref name=steven>{{cite journal|arxiv=1610.05761|bibcode=2017MNRAS.465..403G|doi=10.1093/mnras/stw2708|author1=Steven R. Goldman|author2=Jacco Th. van Loon|title=The wind speeds, dust content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity|year=2016|journal=[[Monthly Notices of the Royal Astronomical Society]]|volume=465|issue=1|pp=403-433}}</ref>}}

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