Lambda Canis Majoris (λ Canis Majoris) is a solitary, blue-white hued star in the constellation Canis Major. Lambda CMa is visible to the naked eye with...
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stars of great distance and high luminosity. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second-brightest star of the constellation and the brightest...
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Theta Canis Majoris (θ Canis Majoris) is a solitary, orange-hued star near the northern edge of the constellation Canis Major, forming the nose of the...
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Omicron1 Canis Majoris (ο1 CMa, ο1 Canis Majoris) is a red supergiant star in the constellation Canis Major. It is also a variable star. Johann Bayer gave...
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Balona, L. A.; Feast, M. W. (1975). "The luminosities of the beta Canis Majoris variables, the zero age main sequence and the distance of the Sco-Cen...
14 KB (1,318 words) - 04:59, 21 August 2024
to 2,000 R☉. Mu Cephei VV Cephei A NML Cygni RW Cephei S Persei VY Canis Majoris - potentially the largest star in the Milky Way KY Cygni PZ Cassiopeiae...
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PC2, HCP and PH3. It was detected in the circumstellar shell of VY Canis Majoris and in the star forming region catalogued as AFGL 5142. The compound...
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B-type supergiant, spectral type B2Ia Omicron² Canis Majoris, B-type supergiant, spectral type B3Ia Lambda Cephei, B-type supergiant, specteal type O6.5I(n)fp...
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{\displaystyle q=2\times 10^{-3}} in the long-period variable M star VY Canis Majoris in the H band, ascribing the CP to multiple scattering in circumstellar...
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system 1.50 Epsilon Canis Majoris Binary star system 1.58 Castor Sextenary star system Brightest sextuple star system 1.62 Lambda Scorpii Triple star...
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direction opposite of the solar apex, is located near the star Zeta Canis Majoris. Animations of star motions around apex and antapex The movement of...
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1889 1889 Amapá Beta Canis Majoris (Mirzam) Canis Major, the Great Dog 2 1991 1992 Rondônia Gamma Canis Majoris (Muliphen) Canis Major, the Great Dog...
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Omicron Puppis (category Lambda Eridani variables)
asterism consisting of ο Puppis, δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, k Puppis, ε Canis Majoris, κ Canis Majoris and π Puppis. Consequently,...
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the View (of the Lion) الطرف الطَّرْف Lambda Leonis Aludra al-ʽUdhrah Virginity العذرة العُذْرَة Eta Canis Majoris Alula Australis, Alula Borealis (al-Qafzat)...
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naked eye examples include Polaris, Alpha Leporis, Alpha Persei, Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars, mostly pulsating...
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sometimes used for the most extended and unstable red supergiants like VY Canis Majoris and NML Cygni. The "red" part of "red supergiant" refers to the cool...
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have been very massive Population III stars. Such stars would dwarf VY Canis Majoris, Mu Cephei and RSGC1-F01, four among the largest known modern stars...
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/ˈæltərf/ Canis Major η Canis Majoris Aludra /əˈluːdrə/ Ursa Major ξ Ursae Majoris Aa Alula Australis /əˈluːlə ɔːˈstreɪlᵻs/ Ursa Major ν Ursae Majoris Alula...
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relatively short period of astronomical time. Very large stars like VY Canis Majoris, one of the largest stars known, together with NML Cygni, VX Sagittarii...
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exoplanets. XO-2N 490 ± 1 2 K0V + K0V 11.18±0.03 Has four exoplanets. Beta Canis Majoris (Mirzam) 490 ± 20 1 B1 II-III 1.985 One of the closest supernova candidates...
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slowed by tidal braking. The best-known metallic-line star is Sirius (α Canis Majoris). The following table lists some metallic-line stars in order of descending...
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HR 2501 (category Lambda Eridani variables)
also known as HD 49131 and HP Canis Majoris, is a star about 2,000 light years from the Earth, in the constellation Canis Major. It is a 5th magnitude...
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Orionis B2Ib – 9 Cephei B3V – Eta Ursae Majoris B3V – Eta Aurigae B3Ia – Omicron2 Canis Majoris B5Ia – Eta Canis Majoris B8Ia – Rigel A-type stars are among...
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giants include: Canopus Albireo Epsilon Canis Majoris Theta Scorpii Beta Draconis Alpha Herculis Gamma Canis Majoris Within any giant luminosity class, the...
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Arietis Pulsar Eclipsing binary Algol variable Beta Lyrae variable W Ursae Majoris variable Supernova Classes Type Ia supernova Type Ib and Ic supernovae...
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disks and increase in brightness are known as shell events. 27 Canis Majoris Beta Canis Minoris Pleione Labadie-Bartz, Jonathan; Baade, Dietrich; Carciofi...
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"Fundamental properties and atmospheric structure of the red supergiant VY Canis Majoris based on VLTI/AMBER spectro-interferometry". Astronomy and Astrophysics...
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V1365 Aquilae V1366 Aquilae NSV 25875 W43A S Persei VX Sagittarii VY Canis Majoris AH Scorpii MY Cephei PZ Cassiopeiae IRC −30308 NML Cygni IRC +10420...
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Beta Centauri (B1III); Mimosa (B0.5III); Bellatrix (B2III); Epsilon Canis Majoris (B2II); and Alpha Lupi (B1.5III) among others. The name blue giant is...
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Current distance Current magnitude Epsilon Canis Majoris ... −4,460,000 −4,700,000 −3.99 34 430 1.50 Beta Canis Majoris −4,460,000 −3,700,000 −4,420,000 −3.65...
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