Abstract
The radial flow of an inviscid heat conducting gas, with gravitational effects, is considered. The gas is assumed non-monatomic, but the limit to the monatomic state is considered in great detail. It is shown that the results of Roberts & Soward (1972) can be predicted from the present analysis, and further that considerable light is shed on their results. For the non-monatomic gas, the various asymptotic regions (obtained when the energy flux at infinity approaches zero) are far simpler in their details than those encountered by Roberts & Soward.
Reference3 articles.
1. Chamberlain J. W. 1961
2. Durney B. 1971 Astrophys.
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