New line blanketed atmosphere models for O type stars

Details New line blanketed atmosphere models for O type stars New line blanketed atmosphere models for O type stars

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..189m&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

One of the main research axis in the modelling of stellar atmospheres of massive stars is the treatment of line blanketing in non-LTE models with stellar winds. We present here the first results of such a modelling obtained with the "comoving frame" code CMFGEN (Hillier & Miller 1999) which includes a more complete treatment of blanketing than our earlier CoStar models (Schaerer & de Koter 1997). We especially focus on the implications of line blanketing on the relation between effective temperature and spectral types for O stars.

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