Krishna Swamy, K. S. (1967) Comparison of the convective model atmospheres of epsilon Eridani and Gmb 1830 The Astrophysical Journal, 150 . pp. 1161-1165. ISSN 0004-637X
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Official URL: http://iopscience.iop.org/0004-637X
Related URL: http://dx.doi.org/10.1086/149412
Abstract
The onset of convection at small optical depth in a metal-deficient star is shown to arise as a result of the decrease in the adiabatic temperature gradient because of the dissociation of the hydrogen molecules and to a steep increase in the radiative temperature gradient brought about as a result of the increase in opacity.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to American Astronomical Society. |
| ID Code: | 87608 |
| Deposited On: | 20 Mar 2012 14:23 |
| Last Modified: | 20 Mar 2012 14:23 |
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