A relaxation method for the computation of model stellar atmospheres-Reference-Cited by-同舟云学术

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A relaxation method for the computation of model stellar atmospheres

Published:1969-06 Issue:2 Volume:4 Page:182-212
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Price Michael J.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00650951.pdf

Reference20 articles.

1. Allen, C. W.: 1963,Astrophysical Quantities, 2nd ed., Athlone Press, London, p. 42.

2. Cilli�, G.: 1932,Monthly Notices Roy. Astron. Soc. 92, 820.

3. Feautrier, P.: 1968, inProc. 3rd Harvard-Smithsonian Conf. Stellar Atmospheres, 1968 (in press).

4. Fleck, J. A. Jr.: 1963,Methods in Computational Physics,I, Academic Press, New York, p. 43.

5. Griem, H. R.: 1960,Astrophys. J. 132, 883.

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1. CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer;Astronomy & Astrophysics;2020-09

2. Monte Carlo Simulations of Radiative and Neutrino Transport under Astrophysical Conditions;Astronomy Reports;2018-05

3. Theory of Stellar Atmospheres;Transactions of the International Astronomical Union Volume XVA;1973

4. Solution of non-LTE transfer problems;Journal of Quantitative Spectroscopy and Radiative Transfer;1971-06

5. The Monte Carlo technique applied to radiative transfer;Journal of Quantitative Spectroscopy and Radiative Transfer;1969-12

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