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- ...Therefore, stars with other luminosity classes can sometimes be considered supergiants. ...s |date=August 2005 |title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought |journal=The Astrophysical Journal |vo ...60 KB (7,829 words) - 18:30, 22 January 2025
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- ...iants at low metallicity: Detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud|journal=Monthly Notices of the Royal Astronom ...t2=Smith |first2=Nathan |title=The Extreme Scarcity of Dust-enshrouded Red Supergiants: Consequences for Producing Stripped Stars via Winds |journal=The Astrophys ...6 KB (783 words) - 01:49, 10 December 2024
- ...018>{{cite thesis|doi=10.11606/D.14.2019.tde-12092018-161841|title=The Red Supergiants in the Supermassive Stellar Cluster Westerlund 1|year=2019|last1=Arévalo|fi ...f Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters|journal=The Astrophysical Journal|volume=7 ...6 KB (874 words) - 21:32, 29 July 2024
- ...lity of Evolved Massive Stars with TESS II: A New Class of Cool, Pulsating Supergiants|journal=The Astrophysical Journal|year=2020|volume=902|issue=1|page=24|doi= ...secs]]. It is one of the [[list of most luminous stars|most luminous]] red supergiants with a luminosity over 250,000 times greater than the Sun ({{Solar luminosi ...8 KB (1,066 words) - 14:15, 27 October 2024
- ...inous Blue Variables, Candidate LBVs, Fe II Emission Line Stars, and Other Supergiants |year=2014 |author-link1=Roberta M. Humphreys|last1=Humphreys |first1=Rober ...INOUS BLUE VARIABLES, CANDIDATE LBVs, Fe II EMISSION LINE STARS, AND OTHER SUPERGIANTS |journal=The Astrophysical Journal |volume=790 |issue=1 |pages=48 |doi=10.1 ...6 KB (793 words) - 16:49, 18 July 2024
- ...A..80F|arxiv=1207.0308|title=Quantitative spectroscopy of Galactic BA-type supergiants. I. Atmospheric parameters|journal=Astronomy & Astrophysics|volume=543|page ...OB stars in the Galaxy. IV. Stellar and wind parameters of early to late B supergiants|journal=Astronomy and Astrophysics|volume=478|issue=3|pages=823|last1=Marko ...6 KB (790 words) - 03:45, 17 July 2024
- ...018>{{cite thesis|doi=10.11606/D.14.2019.tde-12092018-161841|title=The Red Supergiants in the Supermassive Stellar Cluster Westerlund 1|year=2019|last1=Arévalo|fi ...f Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters|journal=The Astrophysical Journal|volume=7 ...7 KB (1,010 words) - 21:32, 29 July 2024
- ...ce Scale|volume=635|pages=149–174|last1=Bresolin|first1=Fabio|chapter=Blue Supergiants as a Tool for Extragalactic Distances — Empirical Diagnostics |year=2003|do ...es of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants |journal=American Astronomical Society Meeting Abstracts |bibcode=2023AAS.. ...10 KB (1,416 words) - 21:27, 16 July 2024
- ...8>{{cite thesis |doi=10.11606/D.14.2019.tde-12092018-161841 |title=The Red Supergiants in the Supermassive Stellar Cluster Westerlund 1 |year=2019 |last1=Arévalo ...ters make W26 one of the [[List of most luminous stars|most luminous]] red supergiants and are similar to those estimated for another notable red supergiant star, ...16 KB (2,255 words) - 20:28, 10 January 2025
- ...= 10.1086/430901 | title = The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool as We Thought | journal = The Astrophysical Journal ...{cite journal|bibcode=2011A&A...526A.156M|title=The mass-loss rates of red supergiants and the de Jager prescription|journal=Astronomy and Astrophysics|volume=526 ...12 KB (1,627 words) - 22:37, 11 February 2025
- ...-AGB star luminosity range and in that of the more massive, younger yellow supergiants.<ref name="parthasarathy" /> [[Stellar spectrum|Spectral]] indicators of l [[Category:G-type supergiants]] ...7 KB (944 words) - 18:57, 23 February 2025
- ...1cbd |title=A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2 |year=2019 |last1=Messineo |first1=M. |last2=Brown |first2=A. G | title=Masses and luminosities of O- and B-type stars and red supergiants ...9 KB (1,170 words) - 20:45, 16 July 2024
- [[Category:G-type supergiants]] [[Category:K-type supergiants]] ...12 KB (1,731 words) - 00:12, 22 June 2024
- | title=Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into T<sub>e | title=Masses and luminosities of O- and B-type stars and red supergiants ...10 KB (1,221 words) - 01:50, 12 October 2024
- ...18|title=Luminosities and mass-loss rates of Local Group AGB stars and Red Supergiants|journal=[[Astronomy & Astrophysics]]|volume=609|pages=A114|doi=10.1051/0004 ...theoretical models of the coolest, most luminous and largest possible cool supergiants (e.g. the [[Hayashi limit]] or the [[Humphreys–Davidson limit]]).<ref name= ...21 KB (3,012 words) - 20:01, 23 February 2025
- ...ng formed from the same star formation burst as that which created the red supergiants in the area. The star is also located about 14 arcminutes from RSGC2, so th ...5 KB (649 words) - 06:15, 4 June 2023
- [[Category:O-type supergiants]] ...4 KB (599 words) - 14:56, 9 October 2024
- ...y the [[CHARA array]] in order to understand the surface variations of red supergiants.<ref name="ryanp"/> ...ct images of the star and test models of 3D radiative hydrodynamics in red supergiants. ...24 KB (3,291 words) - 22:29, 28 February 2025
- ...=2005ApJ...628..973L|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought|journal=The Astrophysical Journal|volu [[Category:M-type supergiants]] ...10 KB (1,434 words) - 10:15, 17 February 2025
- ...st and have spectral features that resemble F- or G-type [[Supergiant star|supergiants]] during the maximum. The outer parts of FU Orionis stars produce a K-M sup [[Category:G-type supergiants]] ...11 KB (1,607 words) - 18:34, 20 October 2024
- ...rage for massive stars in the SMC. However, it is not exceptional for red supergiants, which are believed to show additional extinction due to circumstellar dust ...al|bibcode=2015A&A...578A...3G|arxiv=1504.00003|title=A new survey of cool supergiants in the Magellanic Clouds|journal=Astronomy & Astrophysics|volume=578|pages= ...17 KB (2,439 words) - 19:04, 25 February 2025