Chandrasekhar, S. (1939) The Internal constitution of the stars Proceedings of the American Philosophical Society, 81 (2). pp. 153-187. ISSN 0003-049X
Full text not available from this repository.
Official URL: http://www.jstor.org/pss/984981
Abstract
In This paper an attempt is made to describe the general methods that have been developed to determine the physical conditions in stellar interiors. In view of the complexity of the problem, it is of value to consider, in the first instance, only those methods which involve the minimum of assumptions. Three such methods have been developed in recent years. They are I. The method of the integral theorems. II. The method of the homologous transformations. III. The method of stellar envelopes.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to The American Philosophical Society. |
| ID Code: | 70609 |
| Deposited On: | 22 Nov 2011 03:54 |
| Last Modified: | 22 Nov 2011 03:54 |
Repository Staff Only: item control page
