Abstract
view Abstract Citations (35) References (24) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The effective temperature, radius, rate of mass loss and luminosity of P Cygni, HD 190603, kappa Cassiopeiae, and rho Leonis. Underhill, A. B. Abstract The method developed by Underhill et al. (1979) is applied to P Cyg (B1 Iap), HD 190603 (B1 Ia+), kappa Cas (B1 Ia), and rho Leo (B1 Ib or Iab) using the S2/68 absolute UV photometry for faint stars (Thompson et al., 1978) and the 13-color photometry. Some profiles of the UV resonance lines are presented, and the implication of pertinent data for the interpretation of the observed UV spectrum of the winds from these stars is discussed. Publication: The Astrophysical Journal Pub Date: December 1979 DOI: 10.1086/157526 Bibcode: 1979ApJ...234..528U Keywords: B Stars; Stellar Atmospheres; Stellar Luminosity; Stellar Mass Ejection; Stellar Temperature; Supergiant Stars; Early Stars; Line Spectra; Mass Flow Rate; Radii; Ultraviolet Astronomy; Astrophysics; Diameters:Supergiants; Effective Temperatures:Supergiants; Luminosities:Supergiants; Mass Loss:Supergiants; Supergiants:UV Spectra full text sources ADS | data products SIMBAD (5) MAST (1) INES (1) Related Materials (1) Erratum: 1980ApJ...239..414U
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