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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

Jadwiga Daszyńska-Daszkiewicz  and
Ewa Niemczura
Jadwiga Daszyńska-Daszkiewicz
Affiliation:
Astronomical Institute of the Wrocław University, ul. Kopernika 11, 51-622 Wrocław, Poland Instituut voor Sterrenkunde, Celestijnenlaan 200 B, B-3001 Leuven, Belgium
Ewa Niemczura
Affiliation:
Astronomical Institute of the Wrocław University, ul. Kopernika 11, 51-622 Wrocław, Poland

Abstract

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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

References

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