• V354 Cephei is a red supergiant star located within the Milky Way. It is an irregular variable located over 13,000 light-years away from the Sun. It has...
    13 KB (1,460 words) - 20:33, 14 September 2024
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    hypergiant, together with the red supergiants Mu Cephei, MY Cephei, VV Cephei, V381 Cephei, and V354 Cephei are among the largest stars known. In addition...
    21 KB (2,290 words) - 21:09, 28 July 2024
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    Tsuji, T. (2000). "Water on the Early M Supergiant Stars α Orionis and μ Cephei". The Astrophysical Journal. 538 (2): 801–07. Bibcode:2000ApJ...538..801T...
    174 KB (18,519 words) - 13:39, 13 September 2024
  • 000 3,350 M2-M4 HD 143183 254,000 3,605 M3 LMC 145013 251,000 - 339,000 3,950 M2.5Ia–Ib LMC 25320 251,000 3,800 M V354 Cephei 250,000 3,615 M1Ia-M3.5Ib...
    31 KB (3,277 words) - 10:08, 14 September 2024
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    Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements can be inconsistent...
    235 KB (10,313 words) - 00:32, 15 September 2024
  • Piscium, Nu Eridani, Gamma Pegasi, HD 13745 (V354 Persei) and 53 Arietis had been found to exhibit both Beta Cephei and SPB variability. In 2021 β Cru became...
    27 KB (1,961 words) - 14:46, 17 July 2024
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    cool supergiants and hypergiants such as V509 Cassiopeiae (HR 8752) and RW Cephei. "Ass Cep OB 1". SIMBAD. Centre de données astronomiques de Strasbourg....
    3 KB (197 words) - 03:06, 15 August 2024
  • Size comparison of Betelgeuse, Mu Cephei, KY Cygni, and V354 Cephei according to Emily Levesque's publication...
    12 KB (979 words) - 23:31, 28 July 2024
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    Size comparison of Betelgeuse, Mu Cephei, KY Cygni, and V354 Cephei, according to estimates derived in 2005...
    10 KB (982 words) - 13:50, 5 June 2024
  • and most luminous galactic red supergiants, which includes V354 Cephei, KY Cygni and Mu Cephei. More recently, KW Sagittarii was calculated to have a lower...
    11 KB (1,041 words) - 00:29, 22 July 2024
  • +73° 40′ 27.1″ 10.35 A2IVe UX Ori star, Vmax = 10.35m, Vmin = 12.15m V354 Cephei V354 22h 33m 35s +58° 53′ 45″ 10.90 9000 M2.5 Iab One of the largest known...
    40 KB (125 words) - 19:32, 28 July 2024
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    Piscium, Nu Eridani, Gamma Pegasi, HD 13745 (V354 Persei) and 53 Arietis had been found to exhibit both Beta Cephei and SPB variability. The following list...
    10 KB (689 words) - 19:11, 12 August 2023