Zoznam najväčších hviezd: Rozdiel medzi revíziami
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Riadok 33:
{| class="wikitable"
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! width=226px | Názov hviezdy
! width=167px | Polomer<br /> ([[Slnko]] = 1)
! Metóda
! Poznámky
Riadok 40:
| [[Stephenson 2-18]] || 2 150<ref name="thomas">{{Cite journal|last1=Fok|first1=Thomas K. T|last2=Nakashima|first2=Jun-ichi|last3=Yung|first3=Bosco H. K|last4=Hsia|first4=Chih-Hao|last5=Deguchi|first5=Shuji|year=2012|title=Maser Observations of Westerlund 1 and Comprehensive Considerations on Maser Properties of Red Supergiants Associated with Massive Clusters|journal=The Astrophysical Journal|volume=760|issue=1|pages=65|arxiv=1209.6427|bibcode=2012ApJ...760...65F|doi=10.1088/0004-637X/760/1/65|s2cid=53393926}}</ref> || L/T<sub>eff</sub> || Nachádza sa v masívnej otvorenej hviezdokope [[Stephenson 2]]
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| [[LGGS J004539.99+415404.1]] || 1 980<ref name="massey2016">{{cite journal|doi=10.3847/0004-637X/826/2/224|title=The Red Supergiant Content of M31|journal=The Astrophysical Journal|volume=826|issue=2|pages=224|year=2016|last1=Massey|first1=Philip|last2=Evans|first2=Kate Anne|arxiv=1605.07900|bibcode=2016ApJ...826..224M|s2cid=27871527}}</ref> (– 2 377<ref name="gordon">{{Cite journal|last1=Gordon|first1=Michael S.|last2=Humphreys|first2=Roberta M.|last3=Jones|first3=Terry J.|date=July 2016|title=Luminous and Variable Stars in M31 and M33. III. The Yellow and Red Supergiants and Post-red Supergiant Evolution|journal=The Astrophysical Journal|language=en|volume=825|issue=1|pages=50|doi=10.3847/0004-637X/825/1/50|arxiv=1603.08003|bibcode=2016ApJ...825...50G|s2cid=119281102|issn=0004-637X}}</ref>) || L/T<sub>eff</sub> || Nachádza sa v [[Andromeda (galaxia)|Galaxii Andromeda]]
|-style="background:Gold;" class="sortbottom"
| [[Saturn|Obežná dráha Saturnu]] || 1 940 – 2 169 || – || <small>Uvedené pre porovnanie</small>
|-
| [[MSX LMC 597]] ''(W60 A27)'' || 1 882 – 1 953<ref name=jones>{{Cite journal|last1=Jones|first1=O. C.|last2=Woods|first2=P. M.|last3=Kemper|first3=F.|last4=Kraemer|first4=K. E.|last5=Sloan|first5=G. C.|last6=Srinivasan|first6=S.|last7=Oliveira|first7=J. M.|last8=van Loon|first8=J. Th.|last9=Boyer|first9=M. L.|last10=Sargent|first10=B. A.|last11=McDonald|first11=I.|last12=Meixner|first12=M.|last13=Zijlstra|first13=A. A.|last14=Ruffle|first14=P. M. E.|last15=Lagadec|first15=E.|last16=Pauly|first16=T.|last17=Sewiło|first17=M.|last18=Clayton|first18=G. C.|last19=Volk|first19=K.|date=2017-05-08|title=The SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III|arxiv=1705.02709|journal=Monthly Notices of the Royal Astronomical Society|volume=470|issue=3|pages=3250–3282|doi=10.1093/mnras/stx1101|bibcode=2017MNRAS.470.3250J|s2cid=119371839}}</ref> || L/T<sub>eff</sub> || Nachádza sa vo [[Veľký Magellanov mrak|Veľkom Magellanovom mraku]]
|-
| [[LGGS J004520.67+414717.3]] || 1 870<ref name="massey2016" /> (– 2 510<ref name="gordon" />) || L/T<sub>eff</sub> || Nachádza sa v [[Andromeda (galaxia)|Galaxii Andromeda]]
|-
| [[UY Scuti]] || 1 708 ± 192<ref name="torres2013">{{Cite journal|last1=Arroyo-Torres|first1=B.|last2=Wittkowski|first2=M.|last3=Marcaide|first3=J. M.|last4=Hauschildt|first4=P. H.|title=The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii|doi=10.1051/0004-6361/201220920|journal=Astronomy & Astrophysics|volume=554|pages=A76|year=2013|pmid=|pmc=|bibcode=2013A&A...554A..76A|arxiv=1305.6179}}</ref> || AD || Táto hodnota bola stanovená na základe zdanlivých rozmerov a vzdialenosti hviezdy. Odhad stanovený pomocou družice [[Gaia (satelit)|Gaia]] je však len 755 R<sub>⊙</sub>.<ref name="messineo2019">{{cite journal |bibcode=2019AJ....158...20M |title=A Catalog of Known Galactic K-M Stars of Class I Candidate Red Supergiants in Gaia DR2 |last1=Messineo |first1=M. |last2=Brown |first2=A. G. A. |journal=The Astronomical Journal |year=2019 |volume=158 |issue=1 |pages=20 |doi=10.3847/1538-3881/ab1cbd |arxiv=1905.03744 }}</ref> Avšak paralaxa nameraná družicou Gaia býva často menej presná kvôli astrometrickému rušeniu.<ref name="gaia">{{cite journal
Řádek 58 ⟶ 62:
| doi-access=free
}}</ref>
|-
| [[LGGS J003919.11+404319.2]] || 1 685<ref name="massey2021">{{cite journal|last1=Massey|first1=Philip|last2=Kathryn F.|first2=Neugent|last3=Levesque|first3=Emily M.|last4=Drout|first4=Maria R.|last5=Courteau|first5=Stéphane|date=February 2021|title=The Red Supergiant Content of M31 and M33|arxiv=2011.13279|bibcode=2021AJ....161...79M}}</ref> || L/T<sub>eff</sub> || Nachádza sa v [[Andromeda (galaxia)|Galaxii Andromeda]]
|-
| [[WOH S71]] ''(LMC 23095)'' || 1 662<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|pages=403–433|s2cid=11352637}}</ref> – 1 896<ref name="ren">{{Cite journal|last1=Ren|first1=Yi|last2=Jiang|first2=Bi-Wei|date=2020-07-20|title=On the Granulation and Irregular Variation of Red Supergiants|journal=The Astrophysical Journal|language=en|volume=898|issue=1|pages=24|doi=10.3847/1538-4357/ab9c17|arxiv=2006.06605|bibcode=2020ApJ...898...24R|issn=1538-4357|doi-access=free}}</ref>
|-
| [[HV 2242]] ''(WOH S69)'' || 1 645<ref name="ren" /> || L/T<sub>eff</sub> || Nachádza sa vo [[Veľký Magellanov mrak|Veľkom Magellanovom mraku]]
| [[WOH G64]] || 1 540<ref name="Levesque2009">{{cite journal|title=The Physical Properties of the Red Supergiant WOH G64: The Largest Star Known?|journal=Astronomical Journal|author1=Emily M. Levesque|author2=Philip Massey|author3=Bertrand Plez|author4=Knut A. G. Olsen|last-author-amp=yes|volume=137|issue=6|page=4744|date=June 2009|bibcode=2009AJ....137.4744L|doi=10.1088/0004-6256/137/6/4744|arxiv=0903.2260}}</ref> – 2 575<ref name="vanloon">{{cite journal |bibcode=2005A&A...438..273V |arxiv=astro-ph/0504379 |title=An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars |journal=Astronomy and Astrophysics |volume=438 |issue=1 |pages=273–289 |last1=Van Loon|first1=J. Th. |last2=Cioni|first2=M.-R. L. |last3=Zijlstra|first3=A. A. |last4=Loup|first4=C. |year=2005 |doi=10.1051/0004-6361:20042555}}</ref> || L/T<sub>eff</sub>▼
|-
▲| [[WOH G64]] || 1 540<ref name="Levesque2009">{{cite journal|title=The Physical Properties of the Red Supergiant WOH G64: The Largest Star Known?|journal=Astronomical Journal|author1=Emily M. Levesque|author2=Philip Massey|author3=Bertrand Plez|author4=Knut A. G. Olsen|last-author-amp=yes|volume=137|issue=6|page=4744|date=June 2009|bibcode=2009AJ....137.4744L|doi=10.1088/0004-6256/137/6/4744|arxiv=0903.2260}}</ref> (– 2 575<ref name="vanloon">{{cite journal |bibcode=2005A&A...438..273V |arxiv=astro-ph/0504379 |title=An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars |journal=Astronomy and Astrophysics |volume=438 |issue=1 |pages=273–289 |last1=Van Loon|first1=J. Th. |last2=Cioni|first2=M.-R. L. |last3=Zijlstra|first3=A. A. |last4=Loup|first4=C. |year=2005 |doi=10.1051/0004-6361:20042555}}</ref>) || L/T<sub>eff</sub> || Nachádza sa vo [[Veľký Magellanov mrak|Veľkom Magellanovom mraku]]
|-
| [[RW Cephei]] || 1 535<ref name="humphreys">{{cite journal|doi=10.1086/190559|title=Studies of luminous stars in nearby galaxies. I. Supergiants and O stars in the Milky Way|journal=The Astrophysical Journal Supplement Series|volume=38|pages=309|year=1978|last1=Humphreys|first1=R. M.|bibcode=1978ApJS...38..309H}}</ref><ref name="davies">{{cite journal|doi=10.1111/j.1365-2966.2010.16965.x|title=The potential of red supergiants as extragalactic abundance probes at low spectral resolution|journal=Monthly Notices of the Royal Astronomical Society|volume=407|issue=2|pages=1203|year=2010|last1=Davies|first1=Ben|last2=Kudritzki|first2=Rolf-Peter|last3=Figer|first3=Donald F.|bibcode=2010MNRAS.407.1203D|arxiv = 1005.1008 }}</ref>
|-
| [[Westerlund 1-26]] || 1 530 – 1 580<ref name="wright">{{cite journal|last1=Wright|first1=N. J.|last2=Wesson|first2=R.|last3=Drew|first3=J. E.|last4=Barentsen|first4=G.|last5=Barlow|first5=M. J.|last6=Walsh|first6=J. R.|last7=Zijlstra|first7=A.|last8=Drake|first8=J. J.|last9=Eisloffel|first9=J.|last10=Farnhill|first10=H. J.|title=The ionized nebula surrounding the red supergiant W26 in Westerlund 1|journal=Monthly Notices of the Royal Astronomical Society: Letters|date=16 October 2013|volume=437|issue=1|pages=L1–L5|doi=10.1093/mnrasl/slt127|arxiv=1309.4086|bibcode=2014MNRAS.437L...1W}}</ref><br /> (– 2 550<ref name="thomas"
|-
| [[RSGC1]]-F02 || 1 498<ref name="Davies2008">{{Cite journal | last1 = Davies | first1 = B. | last2 = Figer | first2 = D. F. | last3 = Law | first3 = C. J. | last4 = Kudritzki | first4 = R. P. | last5 = Najarro | first5 = F. | last6 = Herrero | first6 = A. | last7 = MacKenty | first7 = J. W. | doi = 10.1086/527350 | title = The Cool Supergiant Population of the Massive Young Star Cluster RSGC1 | journal = The Astrophysical Journal | volume = 676 | issue = 2 | pages = 1016–1028 | year = 2008 | pmid = | pmc = |arxiv = 0711.4757 |bibcode = 2008ApJ...676.1016D }}</ref> || L/T<sub>eff</sub>
Řádek 487 ⟶ 495:
| titul = Gaia DR2 vo VizieR
| dátum prístupu = 14.5.2020
| url = https://vizier.u-strasbg.fr/viz-bin/VizieR?-source=I/345
| poznámka = Poznámka: Paralaxa (ktorá je dôležitá pri určení polomeru hviezdy) nameraná družicou Gaia, býva často menej presná kvôli astrometrickému rušeniu.}}</ref> – 100<ref name="levesqueetal2005" />
|-
| [[RZ Sagittarii]] || {{0}} {{0}}90,77<ref name="Gaia DR2" /> – 363<ref name="debeck" />
| |||