Physical conditions in the convective envelopes of stars

Author:

Castellani Vittorio,Renzini Alvio

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference9 articles.

1. Baker, N., andKippenhahn, R.: 1962,Z. Astrophys. 54, 114.

2. Caloi, V., Firmani, C., Castellani, V., andRenzini, A.: 1968,Mem. Soc. Astron. Ital. 39, 409.

3. Castellani, V., andRenzini, A.: 1968,Astrophys. Space Sci. 2, 83.

4. Claas, W. J.: 1951,Rech. Observ. Utrecht 12, 14.

5. Cox, A. N.: 1965, inStellar Structures (ed. by L. H. Aller & D. B. McLaughlin).

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The structure of late type stars and the Hayashi track;Astrophysics and Space Science;1974-06

2. Generation of the stellar magnetic field by partially ionized convective envelopes. I;Astrophysics;1973

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

4. Physical conditions in the convective envelope of stars;Astrophysics and Space Science;1971-01

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