Hostname: page-component-5c6d5d7d68-tdptf Total loading time: 0 Render date: 2024-08-15T10:11:23.759Z Has data issue: false hasContentIssue false
  • English
  • Français

A Finite Radius Solution for the Polytrope Index 5

Published online by Cambridge University Press:  25 April 2016

J. O. Murphy
J. O. Murphy*
Affiliation:
Department of Mathematics, Monash University
Get access Rights & Permissions [Opens in a new window]

Extract

Polytropic models have played a significant part in the historical development of stellar structure theory and in other related branches of theoretical astronomy such as stellar pulsations and rotation. In modern astronomy polytropic solutions, because of their wide range of density distributions and our ability to introduce them analytically if necessary, now have an acknowledged role in large scale numerical experiments especially during the developmental stages.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 37 - 39
Copyright
Copyright © Astronomical Society of Australia 1980

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Chandrasekhar, S., ‘An Introduction to the Study of Stellar Structure’, University of Chicago Press (1939).Google Scholar
Seidov, Z. F., and Kuzakhmedov, R. Kh., Soviet Astronomy, 21(3), 399 (1977).Google Scholar
Srivastava, S., Astrophys. J., 136, 680 (1962).CrossRefGoogle Scholar