An abundance analysis of slowly pulsating B stars

Details An abundance analysis of slowly pulsating B stars An abundance analysis of slowly pulsating B stars

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coast.150..183b&link_type=abstract

Communications in Astroseismology, Vol. 150, p.183

Statistics

Methodology

5

Scientific paper

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).

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