[en] We present the methodology and the first results of a study aimed to determine in a self-consistent way the physical parameters T_{eff} and log g as well as NLTE abundances of the majority of all confirmed slowly pulsating B stars (hereafter SPBs).
Morel, Thierry ; Katholieke Universiteit Leuven, Departement Natuurkunde en Sterrenkunde, Instituut voor Sterrenkunde, Celestijnenlaan 200D, 3001 Leuven, Belgium
Language :
English
Title :
An abundance analysis of slowly pulsating B stars
Publication date :
01 June 2007
Journal title :
Communications in Asteroseismology
ISSN :
1021-2043
eISSN :
2224-8374
Publisher :
Verlag der Österreichischen Akademie der Wissenschaften, Wien, Austria
