Atmospheres of extreme metal-deficient stars

Krishna Swamy, K. S. (1969) Atmospheres of extreme metal-deficient stars Astrophysics and Space Science, 4 (2). pp. 218-232. ISSN 0004-640X

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Atmospheric models have been constructed for effective temperatures 4000° , 4500° and 5000° and for hydrogen-to-metal ratios of 1, 102, 103 and 104 times the solar values, and for surface gravities of 2×104 and 2×102. The effect of metal deficiency on the atmospheric structure of these stars are studied.

Item Type:Article
Source:Copyright of this article belongs to Springer-Verlag.
ID Code:18254
Deposited On:17 Nov 2010 12:54
Last Modified:17 May 2016 02:59

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