High-temperature (1000–7000 K) collision-induced absorption of H2 pairs computed from the first principles, with application to cool and dense stellar atmospheres

Author:

Borysow Aleksandra,Jørgensen Uffe G.,Fu Yi

Publisher

Elsevier BV

Subject

Spectroscopy,Atomic and Molecular Physics, and Optics,Radiation

Reference28 articles.

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2. Tsuji T. Model atmospheres of M dwarf stars. In: Kumar S, editor. Low luminosity stars. New York, Gordon and Breach Science Publishers, 1969. p. 457–82.

3. Borysow A. Pressure-induced molecular absorption in stellar atmospheres. In: Jorgensen UG, editor. Molecules in the Stellar environment. Lecture Notes in Physics. Berlin: Springer, 1994. p. 209–222.

4. Model atmospheres of cool, low metallicity stars: the importance of collision-induced absorption;Borysow;Astronom Astrophys,1997

5. Rosseland and Planck mean opacities of a zero-metallicity gas;Lenzuni;Astrophys J Suppl Ser,1991

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