A Grid of Non-LTE Line-Blanketed Model Atmospheres of O Stars

Details A Grid of Non-LTE Line-Blanketed Model Atmospheres of O Stars A Grid of Non-LTE Line-Blanketed Model Atmospheres of O Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..288..157l&link_type=abstract

Stellar Atmosphere Modeling, ASP Conference Proceedings, Vol. 288. Abstracts from a conference held 8-12 April 2002 in Tuebingen

Astronomy and Astrophysics

Astronomy

Scientific paper

We have constructed a grid of over 300 NLTE fully-blanketed model atmospheres covering the parameter range of O-type stars at various metallicities. We have assumed a plane-parallel geometry, hydrostatic and radiative equilibria. The models incorporate about 100,000 NLTE atomic levels of over 40 ions of H, He, C, N, O, Ne, Si, P, S, Fe, and Ni, which are grouped into about 900 superlevels. The models will be made publicly available in the coming months.

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