Effects of porosity on emergent synthetic spectra of massive stars in the X-ray domain

Details Effects of porosity on emergent synthetic spectra of massive stars in the X-ray domain Effects of porosity on emergent synthetic spectra of massive stars in the X-ray domain

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011bsrsl..80..155h&link_type=abstract

Société Royale des Sciences de Liège, Bulletin, vol. 80, p. 155-159 (Proceedings of the 39th Liège Astrophysical Colloquium, hel

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Massive stars possess powerful stellar winds. Studies over the last decade, including the analyses of X-ray emission-line profiles, revealed the importance of wind fragmentation and clumping and led to a downwards revision of the mass-loss rates. We present the first results of our code that allows to compare two models of wind fragmentation, and their consequences on the emergent X-ray spectra of massive stars.

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