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Chemical abundances of β Cephei stars from low- and high-resolution UV spectra
Published online by Cambridge University Press: 12 April 2016
Abstract
We determined the stellar parameters (Teff, [m/H], θ) and E(B – V) for all β Cephei stars observed during the IUE satellite mission. All parameters were derived using an algorithmic procedure of fitting theoretical flux distributions (Kurucz 1996) to the IUE observations.
- Type
- Part 4. Early-type stars: B, A and F pulsators
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 259 - 262
- Copyright
- Copyright © Astronomical Society of the Pacific 2004