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St2-18 memiliki ketidakpastian jarak >50%, yang sangat memengaruhi luminositasnya, dan juga ukurannya. Batas teoritis radius bintang adalah 1500-1800 jari-jari matahari, jadi ukuran ini kemungkinan besar tidak benar.
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(2 revisi perantara oleh pengguna yang sama tidak ditampilkan)
Baris 28:
([[Matahari]] = 1)
!Keterangan
|-
|[[Stephenson 2-18]]
|2.150<ref name="thomas"/>
|Bintang terbesar di jagat raya (sebelumnya UY Scuti)
|-Super raksasa merah
|-
|LGGS J004520.67+414717.3
|2.126<ref>{{Cite journal|last=Ren|first=Yi|last2=Jiang|first2=Bi-Wei|date=2020-07-20|title=On the Granulation and Irregular Variation of Red Supergiants|url=https://iopscience.iop.org/article/10.3847/1538-4357/ab9c17|journal=The Astrophysical Journal|language=en|volume=898|issue=1|pages=24|doi=10.3847/1538-4357/ab9c17|issn=1538-4357}}</ref>
|Bintang yang terletak di [[Galaksi Andromeda]]
|-
|[[MY Cephei]]
|2.061<ref>{{Cite journal|last=Humphreys|first=Roberta M.|last2=Helmel|first2=Greta|last3=Jones|first3=Terry J.|last4=Gordon|first4=Michael S.|date=2020-08|title=Exploring the Mass Loss Histories of the Red Supergiants|url=https://ui.adsabs.harvard.edu/abs/2020arXiv200801108H/abstract|journal=arXiv e-prints|language=en|pages=arXiv:2008.01108}}</ref>
|
|-
|[[WY Velorum]] || 2.028<ref>{{Cite journal|last=Cruzalèbes|first=P|last2=Petrov|first2=R G|last3=Robbe-Dubois|first3=S|last4=Varga|first4=J|last5=Burtscher|first5=L|last6=Allouche|first6=F|last7=Berio|first7=P|last8=Hofmann|first8=K-H|last9=Hron|first9=J|date=2019-12-11|title=A catalogue of stellar diameters and fluxes for mid-infrared interferometry★|url=https://academic.oup.com/mnras/article/490/3/3158/5583026|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=490|issue=3|pages=3158–3176|doi=10.1093/mnras/stz2803|issn=0035-8711}}</ref>
|
|-
| [[V838 Monocerotis]] || 1.570 atau 800<ref>[[V838 Monocerotis]]</ref>
|
|-
| [[WOH G64]] || 1.540<ref name="Levesque2009">{{cite web
Baris 55 ⟶ 37:
|accessdate=2010-07 16
}}</ref>
|Mungkin bintang terbesar yang diketahui.<ref name="Levesque2009" /><ref>{{Cite journal|last=Jones|first=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.|date=2017-09|title=The SAGE-Spec Spitzer Legacy program: the life-cycle of dust and gas in the Large Magellanic Cloud. Point source classification – III|url=https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx1101|journal=Monthly Notices of the Royal Astronomical Society|language=en|volume=470|issue=3|pages=3250–3282|doi=10.1093/mnras/stx1101|issn=0035-8711}}</ref><ref>{{Cite journal|last=de Wit|first=S.|last2=Bonanos|first2=A. Z.|last3=Tramper|first3=F.|last4=Yang|first4=M.|last5=Maravelias|first5=G.|last6=Boutsia|first6=K.|last7=Britavskiy|first7=N.|last8=Zapartas|first8=E.|date=2023-01-01|title=Properties of luminous red supergiant stars in the Magellanic Clouds|url=https://ui.adsabs.harvard.edu/abs/2023A&A...669A..86D|journal=Astronomy and Astrophysics|volume=669|pages=A86|doi=10.1051/0004-6361/202243394|issn=0004-6361}}</ref>
|-
|RSGC1-F01
|1.450<ref>{{Cite journal|last=Decin|first=Leen|last2=Richards|first2=Anita M. S.|last3=Marchant|first3=Pablo|last4=Sana|first4=Hugues|date=2024-01|title=ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants|url=http://arxiv.org/abs/2303.09385|journal=Astronomy & Astrophysics|volume=681|pages=A17|doi=10.1051/0004-6361/202244635|issn=0004-6361}}</ref>
|
|-
| [[VY Canis Majoris]] || 1.420<ref>{{Cite journal|last=Wittkowski|first=M.|last2=Hauschildt|first2=P. H.|last3=Torres|first3=B. Arroyo|last4=Marcaide|first4=J. M.|date=2012-04|title=Fundamental properties and atmospheric structure of the red supergiant VY CMa based on VLTI/AMBER spectro-interferometry|url=http://arxiv.org/abs/1203.5194|journal=Astronomy & Astrophysics|volume=540|pages=L12|doi=10.1051/0004-6361/201219126|issn=0004-6361}}</ref><ref>{{Cite journal|last=Gordon|first=Michael S.|last2=Jones|first2=Terry J.|last3=Humphreys|first3=Roberta M.|last4=Ertel|first4=Steve|last5=Hinz|first5=Philip M.|last6=Hoffmann|first6=William F.|date=2019-01-18|title=Thermal Emission in the Southwest Clump of VY CMa|url=https://doi.org/10.3847/1538-3881/aaf5cb|journal=The Astronomical Journal|volume=157|issue=2|pages=57|doi=10.3847/1538-3881/aaf5cb|issn=1538-3881}}</ref>
| [[V354 Cephei]] || 1.520{{Citation needed|date=December 2009}}
|
|-
|[[AH Scorpii]]
| [[KW Sagittarii]] || 1.460{{Citation needed|date=December 2009}}
|1.411<ref name=":1" />
|
|-
|[[S Persei]]
| [[KY Cygni]] || 1.420{{Citation needed|date=December 2009}}
|1.364<ref>{{Cite web|last=Norris|first=Ryan P.|date=2019|title=Seeing Stars Like Never Before: A Long-term Interferometric Imaging Survey of Red Supergiants|url=https://core.ac.uk/download/pdf/225164189.pdf|website=Georgia State University}}</ref>
|
|-
|[[VX Sagittarii]]
| [[VY Canis Majoris]] || 1.420
|1.356<ref>{{Cite journal|last=Tabernero|first=H. M.|last2=Dorda|first2=R.|last3=Negueruela|first3=I.|last4=Marfil|first4=E.|date=2021-02-01|title=The nature of VX Sagitarii - Is it a TŻO, a RSG, or a high-mass AGB star?|url=https://www.aanda.org/articles/aa/abs/2021/02/aa39236-20/aa39236-20.html|journal=Astronomy & Astrophysics|language=en|volume=646|pages=A98|doi=10.1051/0004-6361/202039236|issn=0004-6361}}</ref>–1.480<ref>{{Cite journal|last=Wallström|first=S. H. J.|last2=Danilovich|first2=T.|last3=Müller|first3=H. S. P.|last4=Gottlieb|first4=C. A.|last5=Maes|first5=S.|last6=Sande|first6=M. Van de|last7=Decin|first7=L.|last8=Richards|first8=A. M. S.|last9=Baudry|first9=A.|date=2024-01-01|title=ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA|url=https://www.aanda.org/articles/aa/abs/2024/01/aa47632-23/aa47632-23.html|journal=Astronomy & Astrophysics|language=en|volume=681|pages=A50|doi=10.1051/0004-6361/202347632|issn=0004-6361}}</ref>
|
|-
| [[Mu Cephei]] || 1.259<ref>{{Cite journal|last=Josselin|first=E.|last2=Plez|first2=B.|date=2007-07|title=Atmospheric dynamics and the mass loss process in red supergiant stars|url=http://arxiv.org/abs/0705.0266|journal=Astronomy & Astrophysics|volume=469|issue=2|pages=671–680|doi=10.1051/0004-6361:20066353|issn=0004-6361}}</ref> – 1.420<ref name=":0">{{Cite journal|last=Levesque|first=Emily M.|last2=Massey|first2=Philip|last3=Olsen|first3=K. A. G.|last4=Plez|first4=Bertrand|last5=Josselin|first5=Eric|last6=Maeder|first6=Andre|last7=Meynet|first7=Georges|date=2005-08|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, But Not As Cool As We Thought|url=http://arxiv.org/abs/astro-ph/0504337|journal=The Astrophysical Journal|volume=628|issue=2|pages=973–985|doi=10.1086/430901|issn=0004-637X}}</ref>
| [[VV Cephei|VV Cephei A]] || 1.050<ref>{{cite journal |author=Habets, G. M. H. J.; Heintze, J. R. W. |title=Empirical bolometric corrections for the main-sequence |journal=Astronomy and Astrophysics Supplement |volume=46 |month=November |year=1981 |pages=193–237 |accessdate=2010-03-14 |url=http://adsabs.harvard.edu/abs/1981A&AS...46..193H}} Page 225 "Table IV" #178</ref>–1.900<ref name="Kaler">{{cite web
|title=VV CEP (VV Cephei)
|publisher=University of Illinois
|author=Professor James B. (Jim) Kaler
|url=http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|accessdate=2010-03-15
|archive-date=2009-02-01
|archive-url=https://web.archive.org/web/20090201112518/http://www.astro.uiuc.edu/~kaler/sow/vvcep.html
|dead-url=yes
}}</ref>
|
|-
| [[V354 Cephei]] || 1.245<ref name=":2">{{Cite journal|last=Healy|first=Sarah|last2=Horiuchi|first2=Shunsaku|last3=Molla|first3=Marta Colomer|last4=Milisavljevic|first4=Dan|last5=Tseng|first5=Jeff|last6=Bergin|first6=Faith|last7=Weil|first7=Kathryn|last8=Tanaka|first8=Masaomi|date=2024-03-23|title=Red Supergiant Candidates for Multimessenger Monitoring of the Next Galactic Supernova|url=http://arxiv.org/abs/2307.08785|journal=Monthly Notices of the Royal Astronomical Society|volume=529|issue=4|pages=3630–3650|doi=10.1093/mnras/stae738|issn=0035-8711}}</ref>
| [[Mu Cephei]] || 1.400<ref name="Levesque2005">{{cite web
|title=The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not as Cool As We Thought
|publisher=Astrophysical Journal
|author=E. M. Levesque
|url=http://iopscience.iop.org/0004-637X/628/2/973/fulltext
|accessdate=2010-07 16
}}</ref>
|
|-
|[[WOH S264]]
| [[RW Cephei]] || 1.260–1.610{{Citation needed|date=December 2009}}
|1.210<ref><nowiki>https://arxiv.org/abs/2405.11019</nowiki></ref>
|
|-
|[[MY Cephei]]
| [[Betelgeuse]] ''(Alpha Orionis)'' || 950–1.000<ref>A NEW VLA-HIPPARCOS DISTANCE TO BETELGEUSE AND ITS IMPLICATIONS. Graham M. Harper et al 2008 The Astronomical Journal 135 1430-1440 doi: 10.1088/0004-6256/135/4/1430 [http://www.iop.org/EJ/abstract/1538-3881/135/4/1430/]{{Pranala mati|date=Agustus 2021 |bot=InternetArchiveBot |fix-attempted=yes }}</ref> atau 880–988<ref>Jim Kaler. 2009-06-26. [http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html Betelgeuse ] {{Webarchive|url=https://web.archive.org/web/20081216023607/http://www.astro.uiuc.edu/~kaler/sow/betelgeuse.html |date=2008-12-16 }} "0.047 seconds of arc, from which we find a true radius of between 4.1 (compromise distance) and 4.6 (larger distance) AU, … extended atmosphere, and the pulsations make it difficult to locate an actual "surface" to tell just how large the star actually is. … "size" of the star depends on the color of observation. Long-wave infrared … up to 5 AU and greater, … shorter-wave infrared … 3 AU. … Betelgeuse to be shrinking … not even round, but somewhat oval"</ref>
|1.134<ref>{{Cite journal|last=Beasor|first=Emma R.|last2=Davies|first2=Ben|date=2018-03-01|title=The evolution of red supergiant mass-loss rates|url=https://ui.adsabs.harvard.edu/abs/2018MNRAS.475...55B|journal=Monthly Notices of the Royal Astronomical Society|volume=475|pages=55–62|doi=10.1093/mnras/stx3174|issn=0035-8711}}</ref>
|
|-
|[[HR 5171|V766 Centauri]] Aa
| [[Antares]] ''(Alpha Scorpii)'' || 883<ref name="foot">approximately 800, derived from the 1990 lunar occultation measurement of apparent diameter of 43.1 milliarcsec (up to ±1 milliarcsec error) (http://adsabs.harvard.edu/abs/1990A&A...230..355R page 361) together with 1997 parallax of 5.40 [1.68] milliarcsec ([http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Antares&submit=SIMBAD+search SIMBAD] citing [http://astrobib.u-strasbg.fr:2008/cgi-bin/cdsbib?1997A%26A...323L..49P Hipparcos]{{Pranala mati|date=Maret 2021 |bot=InternetArchiveBot |fix-attempted=yes }}). The parallax gives a derived distance from 460 to 877 light years. This in turn yields an actual diameter from 653 to 1,246 solar radius. An average of 800 is used here.</ref>
|1.060 — 1.160<ref>{{Cite journal|last=van Genderen|first=A. M.|last2=Lobel|first2=A.|last3=Nieuwenhuijzen|first3=H.|last4=Henry|first4=G. W.|last5=de Jager|first5=C.|last6=Blown|first6=E.|last7=Di Scala|first7=G.|last8=van Ballegoij|first8=E. J.|date=2019-11|title=Pulsations, eruptions, and evolution of four yellow hypergiants|url=http://arxiv.org/abs/1910.02460|journal=Astronomy & Astrophysics|volume=631|pages=A48|doi=10.1051/0004-6361/201834358|issn=0004-6361}}</ref>
|
|-
| [[UYKY ScutiCygni]] || 755
|1.033<ref>{{Cite journal|last=Comerón|first=F.|last2=Djupvik|first2=A. A.|last3=Schneider|first3=N.|last4=Pasquali|first4=A.|date=2020-12-01|title=The historical record of massive star formation in Cygnus|url=https://ui.adsabs.harvard.edu/abs/2020A&A...644A..62C|journal=Astronomy and Astrophysics|volume=644|pages=A62|doi=10.1051/0004-6361/202039188|issn=0004-6361}}</ref>
|
|-
| [[KW Sagittarii]]|| 1.009 ± 142<ref name=":1">{{Cite journal|last=Arroyo-Torres|first=B.|last2=Wittkowski|first2=M.|last3=Marcaide|first3=J. M.|last4=Hauschildt|first4=P. H.|date=2013-06|title=The atmospheric structure and fundamental parameters of the red supergiants AH Sco, UY Sct and KW Sgr|url=http://arxiv.org/abs/1305.6179|journal=Astronomy & Astrophysics|volume=554|pages=A76|doi=10.1051/0004-6361/201220920|issn=0004-6361}}</ref>
| [[V382 Carinae]] || 747
|
|-
| [[UY Scuti]]|| 909<ref name=":2" />
|
|-
|[[VV Cephei|VV Cephei A]]
|779.27<ref>{{Cite journal|last=Baines|first=Ellyn K.|last2=Armstrong|first2=J. Thomas|last3=Clark|first3=James H.|last4=Gorney|first4=Jim|last5=Hutter|first5=Donald J.|last6=Jorgensen|first6=Anders M.|last7=Kyte|first7=Casey|last8=Mozurkewich|first8=David|last9=Nisley|first9=Ishara|date=2021-10|title=Angular Diameters and Fundamental Parameters of Forty-four Stars from the Navy Precision Optical Interferometer|url=https://dx.doi.org/10.3847/1538-3881/ac2431|journal=The Astronomical Journal|language=en|volume=162|issue=5|pages=198|doi=10.3847/1538-3881/ac2431|issn=1538-3881}}</ref>
|
|-
| [[RW Cephei]] || 900–1760<ref>{{Cite journal|last=Anugu|first=Narsireddy|last2=Baron|first2=Fabien|last3=Gies|first3=Douglas R.|last4=Lanthermann|first4=Cyprien|last5=Schaefer|first5=Gail H.|last6=Shepard|first6=Katherine A.|last7=Brummelaar|first7=Theo ten|last8=Monnier|first8=John D.|last9=Kraus|first9=Stefan|date=2023-07|title=The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis|url=https://dx.doi.org/10.3847/1538-3881/ace59d|journal=The Astronomical Journal|language=en|volume=166|issue=2|pages=78|doi=10.3847/1538-3881/ace59d|issn=1538-3881}}</ref>
|
|-
| [[Betelgeuse]] ''(Alpha Orionis)''|| 764<ref>{{Cite journal|last=Joyce|first=Meridith|last2=Leung|first2=Shing-Chi|last3=Molnár|first3=László|last4=Ireland|first4=Michael|last5=Kobayashi|first5=Chiaki|last6=Nomoto|first6=Ken'ichi|date=2020-10-01|title=Standing on the Shoulders of Giants: New Mass and Distance Estimates for Betelgeuse through Combined Evolutionary, Asteroseismic, and Hydrodynamic Simulations with MESA|url=https://ui.adsabs.harvard.edu/abs/2020ApJ...902...63J|journal=The Astrophysical Journal|volume=902|pages=63|doi=10.3847/1538-4357/abb8db|issn=0004-637X}}</ref>
|bintang paling terang ke-10 di langit malam.
|-
| [[Antares]] ''(Alpha Scorpii)'' || 680<ref>{{Cite journal|last=Ohnaka|first=Keiichi|last2=Hofmann|first2=Karl-Heinz|last3=Schertl|first3=Dieter|last4=Weigelt|first4=Gerd|last5=Baffa|first5=Carlo|last6=Chelli|first6=Alain|last7=Petrov|first7=Romain|last8=Robbe-Dubois|first8=Sylvie|date=2013-07|title=High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER|url=http://arxiv.org/abs/1304.4800|journal=Astronomy & Astrophysics|volume=555|pages=A24|doi=10.1051/0004-6361/201321063|issn=0004-6361}}</ref>
|bintang paling terang ke-15 di langit malam.
|-
|[[Rho Cassiopeiae]]
|636–981<ref>{{Cite journal|last=van Genderen|first=A. M.|last2=Lobel|first2=A.|last3=Nieuwenhuijzen|first3=H.|last4=Henry|first4=G. W.|last5=de Jager|first5=C.|last6=Blown|first6=E.|last7=Di Scala|first7=G.|last8=van Ballegoij|first8=E. J.|date=2019-11-01|title=Pulsations, eruptions, and evolution of four yellow hypergiants|url=https://ui.adsabs.harvard.edu/abs/2019A&A...631A..48V|journal=Astronomy and Astrophysics|volume=631|pages=A48|doi=10.1051/0004-6361/201834358|issn=0004-6361}}</ref>
|
|-
Baris 108 ⟶ 106:
|
|-
| [[{{ill|T Cephei]] |en}}|| 540<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9837</ref>
|
|-
Baris 114 ⟶ 112:
|
|-
| [[{{ill|W Hydrae]] |en}}|| 520<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=6127</ref>
|
|-
| [[{{Ill|R Cassiopeiae]] |en}}|| 500<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=10947</ref>
|
|-
| [[V382 Carinae]] || 485<ref>{{Cite journal|last=Groenewegen|first=M. A. T.|date=2020-03|title=Analysing the spectral energy distributions of Galactic classical Cepheids|url=http://arxiv.org/abs/2002.02186|journal=Astronomy & Astrophysics|volume=635|pages=A33|doi=10.1051/0004-6361/201937060|issn=0004-6361}}</ref>
| [[Chi Cygni]] || 470<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107</ref>
|Hypergiant paling terang di langit.
|
|-
| {{ill|Chi Cygni|en}} || 470<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=9107</ref>
| [[Alpha Herculis]] ''(Ras Algethi)'' || 460
|
|-
| [[V838 Monocerotis]]|| 467<ref>{{Cite journal|last=Kamiński|first=Tomek|last2=Tylenda|first2=Romuald|last3=Kiljan|first3=Aleksandra|last4=Schmidt|first4=Mirek|last5=Lisiecki|first5=Krzysztof|last6=Melis|first6=Carl|last7=Frankowski|first7=Adam|last8=Joshi|first8=Vishal|last9=Menten|first9=Karl M.|date=2021-11-01|title=V838 Monocerotis as seen by ALMA: A remnant of a binary merger in a triple system|url=https://ui.adsabs.harvard.edu/abs/2021A&A...655A..32K|journal=Astronomy and Astrophysics|volume=655|pages=A32|doi=10.1051/0004-6361/202141526|issn=0004-6361}}</ref>
| [[Rho Cassiopeiae]] || 450
|
|-
| [[Mira|Mira A]] ''(Omicron Ceti)'' || 400<ref>http://www.eso.org/~mwittkow/publications/conferences/SPIECWo5491199.pdf</ref>
Baris 146 ⟶ 145:
| accessdate=2009-03-25 | bibcode=1995ASPC...83..176L
}}</ref>
|
|-
| [[R Doradus]] || 370
|
|-
Baris 154 ⟶ 150:
|
|-
| [[R Doradus]] || 298 ± 21<ref>{{Cite journal|last=Ohnaka|first=Keiichi|last2=Weigelt|first2=Gerd|last3=Hofmann|first3=Karl-Heinz|date=2019-09-01|title=Infrared Interferometric Three-dimensional Diagnosis of the Atmospheric Dynamics of the AGB Star R Dor with VLTI/AMBER|url=https://ui.adsabs.harvard.edu/abs/2019ApJ...883...89O|journal=The Astrophysical Journal|volume=883|pages=89|doi=10.3847/1538-4357/ab3d2a|issn=0004-637X}}</ref>
| [[R Leonis]] || 350<ref>http://arxiv.org/abs/astro-ph/0411133</ref>
|
|-
| [[Alpha Herculis]] ''(Ras Algethi)'' || 284 ± 60<ref>{{Cite journal|last=Moravveji|first=Ehsan|last2=Guinan|first2=Edward F.|last3=Khosroshahi|first3=Habib G.|last4=Wasatonic|first4=Rick|date=2013-11-01|title=The Age and The Mass of The \alpha Herculis Triple-Star System From A MESA Grid of rotating stars with 1.3|url=http://arxiv.org/abs/1308.1632|journal=The Astronomical Journal|volume=146|issue=6|pages=148|doi=10.1088/0004-6256/146/6/148|issn=0004-6256}}</ref>
| [[Pistol Star|The Pistol Star]] || 340
|
|-
| [[Eta Carinae]] || 240<ref>{{Cite journal|last=Gull|first=Theodore R.|last2=Damineli|first2=Augusto|date=2009-11|title=Eta Carinae in the Context of the Most Massive Stars|url=http://arxiv.org/abs/0910.3158|journal=Proceedings of the International Astronomical Union|volume=5|issue=H15|pages=373–398|doi=10.1017/S1743921310009890|issn=1743-9213}}</ref> (60 – 881)<ref>{{Cite journal|last=Hillier|first=D. John|last2=Davidson|first2=K.|last3=Ishibashi|first3=K.|last4=Gull|first4=T.|date=2001-06-01|title=On the Nature of the Central Source in η Carinae|url=https://ui.adsabs.harvard.edu/abs/2001ApJ...553..837H|journal=The Astrophysical Journal|volume=553|pages=837–860|doi=10.1086/320948|issn=0004-637X}}</ref>
| [[Alpha Draconis]] ''(Thuban)'' || 265
|
|-
| {{Ill|La Superba|en}}|| 225
| [[119 Tauri]] ''("Ruby Star")''<ref>[http://jumk.de/astronomie/big-stars/119-tauri.shtml "Big and Giant Stars"]</ref> || 255<ref>http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=II/224/cadars&recno=2526</ref>
|
|-
| [[Delta Canis Majoris]] ''(Wezen)'' || 215±66<ref>{{cite journal|last= Davis J, Booth AJ, Ireland MJ, Jacob AP, North JR, Owens SM, Robertson JG, Tango WJ, Tuthill PG|year=2007|first1= J.|pages= 151|last2= Booth|first2= A. J.|last3= Ireland|first3= M. J.|last4= Jacob|first4= A. P.|last5= North|first5= J. R.|last6= Owens|first6= S. M.|last7= Robertson|first7= J. G.|last8= Tango|first8= W. J.|last9= Tuthill|first9= P. G.|volume= 24|title=The Emergent Flux and Effective Temperature of Delta Canis Majoris|journal= Publications of the Astronomical Society of Australia|doi=10.1071/AS07017|url=http://arxiv.org/abs/0709.3873v1|accessdate=28 May 2010}}</ref>
| [[La Superba]] ''([[Y Canum Venaticorum]])'' || 225
|bintang paling terang ke-36 di langit malam.
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|-
| [[Epsilon Pegasi]] ''(Enif)'' || 211<ref>{{Cite journal|last=Stock|first=S.|last2=Reffert|first2=S.|last3=Quirrenbach|first3=A.|date=2018-05-01|title=VizieR Online Data Catalog: Stellar parameters of 372 giant stars (Stock+, 2018)|url=https://ui.adsabs.harvard.edu/abs/2018yCat..36160033S|journal=VizieR Online Data Catalog|pages=J/A+A/616/A33|doi=10.26093/cds/vizier.36160033}}</ref>
| [[Deneb]] ''(Alpha Cygni)'' || 220
|
|-
| [[Deneb]] ''(Alpha Cygni)'' || 203 ± 17<ref>{{Cite journal|last=Schiller|first=Florian|last2=Przybilla|first2=Norbert|date=2008-03|title=Quantitative spectroscopy of Deneb|url=http://arxiv.org/abs/0712.0040|journal=Astronomy & Astrophysics|volume=479|issue=3|pages=849–858|doi=10.1051/0004-6361:20078590|issn=0004-6361}}</ref>
| [[Delta Canis Majoris]] ''(Wezen)'' || 215±66<ref>{{cite journal|last= Davis J, Booth AJ, Ireland MJ, Jacob AP, North JR, Owens SM, Robertson JG, Tango WJ, Tuthill PG|year=2007|first1= J.|pages= 151|last2= Booth|first2= A. J.|last3= Ireland|first3= M. J.|last4= Jacob|first4= A. P.|last5= North|first5= J. R.|last6= Owens|first6= S. M.|last7= Robertson|first7= J. G.|last8= Tango|first8= W. J.|last9= Tuthill|first9= P. G.|volume= 24|title=The Emergent Flux and Effective Temperature of Delta Canis Majoris|journal= Publications of the Astronomical Society of Australia|doi=10.1071/AS07017|url=http://arxiv.org/abs/0709.3873v1|accessdate=28 May 2010}}</ref>
|bintang paling terang ke-19 di langit malam.
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|-
| [[Zeta Aurigae]] || 200<ref>{{Cite web |url=http://www.hposoft.com/EAur09/ZetaAurigae.html |title=Salinan arsip |access-date=2010-10-07 |archive-date=2012-03-21 |archive-url=https://web.archive.org/web/20120321213715/http://www.hposoft.com/EAur09/ZetaAurigae.html |dead-url=yes }}</ref>
|
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| [[Epsilon Aurigae]] A || 143 – 358<ref>{{Cite journal|last=Kloppenborg|first=Brian|last2=Stencel|first2=Robert|last3=Monnier|first3=John D.|last4=Schaefer|first4=Gail|last5=Baron|first5=Fabien|last6=Tycner|first6=Chris|last7=Zavala|first7=Robert T.|last8=Hutter|first8=Donald|last9=Zhao|first9=Ming|date=2015-09-21|title=Interferometry of $\epsilon$ Aurigae: Characterization of the asymmetric eclipsing disk|url=http://arxiv.org/abs/1508.01909|journal=The Astrophysical Journal Supplement Series|volume=220|issue=1|pages=14|doi=10.1088/0067-0049/220/1/14|issn=1538-4365}}</ref>
| [[Eta Carinae]] || 85–195<ref>http://etacar.umn.edu/etainfo/basic/</ref>
|
|-
| [[Epsilon Aurigae]] A || 175
|
|-
| [[Epsilon Carinae]] || 153
|Bintang paling terang ke-39 di langit malam.
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|-
| [[{{Ill|LBV 1806-20]] |en}}|| 150
|
|-
| [[Epsilon Pegasi]] ''(Enif)'' || 150
|
|-
Baris 196 ⟶ 186:
|
|-
| [[Gamma Andromedae]] || 8380
|
|-
| [[Rigel]] ''(Beta Orionis)'' || 78.9<ref>{{Cite journal|last=Moravveji|first=Ehsan|last2=Guinan|first2=Edward F.|last3=Shultz|first3=Matt|last4=Williamson|first4=Michael H.|last5=Moya|first5=Andres|date=2012-03-10|title=Asteroseismology of the Nearby SN-II Progenitor: Rigel Part I. The MOST High Precision Photometry and Radial Velocity Monitoring|url=http://arxiv.org/abs/1201.0843|journal=The Astrophysical Journal|volume=747|issue=2|pages=108|doi=10.1088/0004-637X/747/2/108|issn=0004-637X}}</ref>
| [[Rigel]] ''(Beta Orionis)'' || 78
|Bintang paling terang ke-7 di langit malam.
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| [[Alpha Leporis]] ''(Arneb)'' || 7775
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| [[Canopus]] ''(Alpha Carinae)''|| 73.3<ref>{{Cite journal|last=de Souza|first=A. Domiciano|last2=Zorec|first2=J.|last3=Millour|first3=F.|last4=Bouquin|first4=J.-B. Le|last5=Spang|first5=A.|last6=Vakili|first6=F.|date=2021-10|title=Refined fundamental parameters of Canopus from combined near-IR interferometry and spectral energy distribution|url=http://arxiv.org/abs/2109.07153|journal=Astronomy & Astrophysics|volume=654|pages=A19|doi=10.1051/0004-6361/202140478|issn=0004-6361}}</ref>
| [[R Coronae Borealis]] || 65
|bintang paling terang ke-2 di langit malam.
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| [[Alpha Persei]] ''(Mirfak)''|| 68<ref>{{Cite journal|last=Nordgren|first=Tyler E.|last2=Germain|first2=M. E.|last3=Benson|first3=J. A.|last4=Mozurkewich|first4=D.|last5=Sudol|first5=J. J.|last6=Elias|first6=N. M., II|last7=Hajian|first7=Arsen R.|last8=White|first8=N. M.|last9=Hutter|first9=D. J.|date=1999-12-01|title=Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer|url=https://ui.adsabs.harvard.edu/abs/1999AJ....118.3032N|journal=The Astronomical Journal|volume=118|pages=3032–3038|doi=10.1086/301114|issn=0004-6256}}</ref>
| [[Canopus]] ''(Alpha Carinae)'' || 65
|bintang paling terang ke-35 di langit malam.
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| [[Albireo]] (Beta Cygni Aa'')''|| 62<ref>{{Cite journal|last=Drimmel|first=Ronald|last2=Sozzetti|first2=Alessandro|last3=Schroeder|first3=Klaus-Peter|last4=Bastian|first4=Ulrich|last5=Pinamonti|first5=Matteo|last6=Jack|first6=Dennis|last7=Huerta|first7=Missael A. Hernandez|date=2021-01-28|title=A celestial matryoshka: Dynamical and spectroscopic analysis of the Albireo system|url=http://arxiv.org/abs/2012.01277|journal=Monthly Notices of the Royal Astronomical Society|volume=502|issue=1|pages=328–350|doi=10.1093/mnras/staa4038|issn=0035-8711}}</ref>
| [[Delta Orionis]] ''(Mintaka)'' || 60
|
|-
| [[Zeta Geminorum]] ''(Mekbuda)''|| 65.24<ref>{{Cite journal|last=Groenewegen|first=M. A. T.|date=2007-11-01|title=The projection factor, period-radius relation, and surface-brightness colour relation in classical cepheids|url=https://ui.adsabs.harvard.edu/abs/2007A&A...474..975G|journal=Astronomy and Astrophysics|volume=474|pages=975–981|doi=10.1051/0004-6361:20078225|issn=0004-6361}}</ref>
| [[Alpha Persei]] ''(Mirfak)'' || 60
|
|-
| [[Alpha Hydrae]] ''(Alphard)''|| 50.5<ref>{{Cite journal|last=da Silva|first=L.|last2=Girardi|first2=L.|last3=Pasquini|first3=L.|last4=Setiawan|first4=J.|last5=von der Luhe|first5=O.|last6=de Medeiros|first6=J. R.|last7=Hatzes|first7=A.|last8=Dollinger|first8=M. P.|last9=Weiss|first9=A.|date=2006-11|title=Basic physical parameters of a selected sample of evolved stars|url=http://arxiv.org/abs/astro-ph/0608160|journal=Astronomy & Astrophysics|volume=458|issue=2|pages=609–623|doi=10.1051/0004-6361:20065105|issn=0004-6361}}</ref>
| [[Zeta Geminorum]] ''(Mekbuda)'' || 60
|
|-
| [[Aldebaran]] ''(Alpha Tauri)'' || 43<ref>http://adsabs.harvard.edu/abs/2005astro.ph..2181R</ref>
| [[Eta Aquilae]] || 60
|Bintang paling terang ke-14 di langit malam.
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| [[Gamma{{ill|Beta Draconis]]Ursae Minoris|en}} ''(EltaninKochab)'' || 5041
|
|-
|[[Polaris]]
| [[Aldebaran]] ''(Alpha Tauri)'' || 43<ref>http://adsabs.harvard.edu/abs/2005astro.ph..2181R</ref>
|37.5<ref>{{Cite journal|last=Fadeyev|first=Yu A.|date=2015-05-01|title=Evolutionary status of Polaris|url=http://arxiv.org/abs/1502.06463|journal=Monthly Notices of the Royal Astronomical Society|volume=449|issue=1|pages=1011–1017|doi=10.1093/mnras/stv412|issn=1365-2966}}</ref>
|
|-
|[[Arcturus]]
| [[Beta Ursae Minoris]] ''(Kochab)'' || 41
|25.4<ref>{{Cite journal|last=Ramirez|first=I.|last2=Prieto|first2=C. Allende|date=2011-12-20|title=Fundamental Parameters and Chemical Composition of Arcturus|url=http://arxiv.org/abs/1109.4425|journal=The Astrophysical Journal|volume=743|issue=2|pages=135|doi=10.1088/0004-637X/743/2/135|issn=0004-637X}}</ref>
|
|Bintang paling terang ke-4 di langit malam.
|-
| [[BetaZeta DraconisOrionis]] ''(RastabanAlnitak)'' || 4020
|bintang paling terang ke-32 di langit malam.
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| [[Mintaka]] ''(Delta Orionis)''|| 16.5<ref>{{Cite journal|last=Shenar|first=T.|last2=Oskinova|first2=L.|last3=Hamann|first3=W. -R.|last4=Corcoran|first4=M. F.|last5=Moffat|first5=A. F. J.|last6=Pablo|first6=H.|last7=Richardson|first7=N. D.|last8=Waldron|first8=W. L.|last9=Huenemoerder|first9=D. P.|date=2015-08-01|title=A Coordinated X-Ray and Optical Campaign of the Nearest Massive Eclipsing Binary, δ Orionis Aa. IV. A Multiwavelength, Non-LTE Spectroscopic Analysis|url=https://ui.adsabs.harvard.edu/abs/2015ApJ...809..135S|journal=The Astrophysical Journal|volume=809|pages=135|doi=10.1088/0004-637X/809/2/135|issn=0004-637X}}</ref>
| [[Zeta Orionis]] ''(Alnitak)'' || 20
|
|-
| [[Zeta Puppis]] ''(Naos)''|| 14 – 26<ref>{{Cite journal|last=Schilbach|first=E.|last2=Röser|first2=S.|date=2008-10-01|title=On the origin of field O-type stars|url=https://ui.adsabs.harvard.edu/abs/2008A&A...489..105S|journal=Astronomy and Astrophysics|volume=489|pages=105–114|doi=10.1051/0004-6361:200809936|issn=0004-6361}}</ref>
| [[Zeta Puppis]] ''(Naos)'' || 18.6
|
|-
|[[Beta Geminorum|Pollux]]
| [[Beta Cygni]] A1 ''(Albireo)'' || 16
|9.06<ref>{{Cite journal|last=Baines|first=Ellyn K.|last2=Armstrong|first2=J. Thomas|last3=Schmitt|first3=Henrique R.|last4=Zavala|first4=R. T.|last5=Benson|first5=James A.|last6=Hutter|first6=Donald J.|last7=Tycner|first7=Christopher|last8=van Belle|first8=Gerard T.|date=2017-12-20|title=Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer|url=http://arxiv.org/abs/1712.08109|journal=The Astronomical Journal|volume=155|issue=1|pages=30|doi=10.3847/1538-3881/aa9d8b|issn=1538-3881}}</ref>
|
|Bintang paling terang ke-17 di langit malam.
|-
|[[Sirius]] A
|1.711<ref>{{Cite journal|last=Liebert|first=James|last2=Young|first2=Patrick A.|last3=Arnett|first3=David|last4=Holberg|first4=J. B.|last5=Williams|first5=Kurtis A.|date=2005-09-01|title=The Age and Progenitor Mass of Sirius B|url=http://arxiv.org/abs/astro-ph/0507523|journal=The Astrophysical Journal|volume=630|issue=1|pages=L69–L72|doi=10.1086/462419|issn=0004-637X}}</ref>
|Bintang paling terang di langit malam.
|}
 
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