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Spectroscopy Of Low Metallicity Giant H II Regions: A grid of low Metallicity Stellar atmospheres
S. L. Pistinner, P. H. Hauschildt, D. Eichler +1
We calculate a grid of spherically symmetric OB stellar atmospheres at low metallicities, including both non-local thermodynamic equilibrium (NLTE) and metal line blanketing effect…
Numerical Solution of the Expanding Stellar Atmosphere Problem
P. H. Hauschildt, E. Baron
In this paper we discuss numerical methods and algorithms for the solution of NLTE stellar atmosphere problems involving expanding atmospheres, e.g., found in novae, supernovae and…
The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$
Peter H. Hauschildt, France Allard, E. Baron
We present our NextGen Model Atmosphere grid for low mass stars for effective temperatures larger than $3000\K$. These LTE models are calculated with the same basic model assumptio…
Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams
Isabelle Baraffe, Gilles Chabrier, France Allard +1
We present evolutionary models for low mass stars from 0.075 to 1 $\msol$ for solar-type metallicities [M/H]= 0 and -0.5. The calculations include the most recent interior physics…
A Spherical Non-LTE Line-Blanketed Stellar Atmosphere Model of the Early B Giant epsilon CMa
J. P. Aufdenberg, P. H. Hauschildt, S. N. Shore +1
We use a spherical non-LTE fully line blanketed model atmosphere to fit the full multi-wavelength spectrum, including the extreme ultraviolet (EUV) continuum observed by the {\it E…