[HS80] B157 , the SIMBAD biblio

[HS80] B157 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST02:24:12


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Title First 3 Authors
1993ApJS...89...85I viz 2501 42 A catalog of blue and red supergiants in M33. IVANOV G.R., FREEDMAN W.L. and MADORE B.F.
1995ApJS...99..551H viz 52 11 The massive star populations in ionized gas shells in M33 and M31. HUNTER D.A., BOYD D.M. and HAWLEY W.N.
1996ApJ...469..629M viz 363 89 The UV-brightest stars of M33 and its nucleus: discovery, photometry, and optical spectroscopy. MASSEY P., BIANCHI L., HUTCHINGS J.B., et al.
1997BSAO...43..133F 543 7 Photometry of OB stars on H-alpha images of M33. FABRIKA S.N., SHOLUKHOVA O.N. and ZAKHAROVA S.A.
1999A&AS..140..309F viz 14       D               1 544 7 A survey of blue - Hα objects in the galaxy M 33. FABRIKA S. and SHOLUKHOVA O.
2005ApJ...635..311U 35 59 Blue luminous stars in nearby galaxies: quantitative spectral analysis of M33 B-type supergiant stars. URBANEJA M.A., HERRERO A., KUDRITZKI R.-P., et al.
2006AJ....131.2478M viz 15       D               1 554 395 A survey of Local Group galaxies currently forming stars. I. UBVRI photometry of stars in M 31 and M 33. MASSEY P., OLSEN K.A.G., HODGE P.W., et al.
2007A&A...470..843M 83 65 The building up of the disk galaxy M33 and the evolution of the metallicity gradient. MAGRINI L., CORBELLI E. and GALLI D.
2009ApJ...704.1120U 15       D               2 35 64 A new distance to M33 using blue supergiants and the FGLR method. U V., URBANEJA M.A., KUDRITZKI R.-P., et al.
2017AJ....154...75L 79               F     1 17 1 Extra-galactic distances with massive stars: the role of stellar variability in the case of M33. LEE C.-H.
2019A&A...621A..38G viz 16       D               1 39805 85 The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. GEIER S., RADDI R., GENTILE FUSILLO N.P., et al.
2022ApJS..260...41W viz 17       D               3 156 4 Dust Extinction Law in Nearby Star-resolved Galaxies. II. M33 Traced by Supergiants. WANG Y., GAO J., REN Y., et al.

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