منابع مشابه
The Molecular Line Opacity of MgH in Cool Stellar Atmospheres
A new, complete, theoretical rotational and vibrational line list for the A 2 Π ← X 2 Σ + electronic transition in MgH is presented. The list includes transition energies and oscillator strengths for all possible allowed transitions and was computed using the best available theoretical potential energies and dipole transition moment function with the former adjusted to account for experimental ...
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15 صفحه اولElectronic Structure and Radiative Opacity of the Metallic Elements in Hot and Dense Stellar Material
Electronic structures of the metallic elements in hot and dense stellar material are calculated with an averageatom scheme, which is designed to consider the environmental influence in a mixture. It ensures that all kinds of atoms have the same temperature, the same chemical potential, and the same electron density at the boundaries between the atoms, and that the electrical neutrality within e...
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متن کاملThe Molecular Continuum Opacity of 24 MgH in Cool Stellar Atmospheres
The opacity due to photodissociation of 24 MgH is investigated in the atmospheres of cool stars. The lowest two electronic transitions A 2 Π ← X 2 Σ + and B ′ 2 Σ + ← X 2 Σ + are considered where the cross sections for the latter were published previously (Weck, Stancil, & Kirby 2002a) while the former are presented in this work. Model atmospheres calculated with the PHOENIX code are used to in...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1932
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/92.5.364