Published October 1975
| Version v1
Journal article
Rotational distortion of polytropes by analytic approximation
Description
This paper modifies the first-order perturbation theory of Chandrasekhar, for rotational distortion of polytropes. Comparison with numerical integrations by other authors demonstrates that the present analytic theory is as accurate as other published first-order theories. The present theory is in a form permitting rapid calculation of boundary shapes as a function of the rotation parameter, v, and the polytrope index, n. Results are presented for a critically rotating polytrope, for the case n=3. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00646063;
Publishing Information
- Journal Title
- Astrophysics and Space Science
- Journal Volume
- 37
- Journal Issue
- 1
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 73-86
- ISSN
- 0004-640X
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 7226651
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANALYTICAL SOLUTION; ASTROPHYSICS; CHANDRASEKHAR THEORY; ROTATION; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent