Published August 1972
| Version v1
Journal article
Structure of chemically homogeneous main-sequence stars
Creators
Description
The general dffferential equations for the structure of stars are developed. These are then applied to the analysis of the structure of chemically homogeneous main-sequence stars. Some general deductions are made about the dependence of the slope of the main sequence on the energy generating cycle. The variation in the position of the main sequence with chemical composition is also discussed. Key words: stellar structure - stellar models
Additional details
Identifiers
- DOI
- 10.1086/129319;
Publishing Information
- Journal Title
- Publications of the Astronomical Society of the Pacific
- Journal Volume
- 84
- Journal Issue
- 500
- Series
- Publ. Astron. Soc. Pac.
- Journal Page Range
- 465
- ISSN
- 0004-6280
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 4052198
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CHEMICAL COMPOSITION; DIFFERENTIAL EQUATIONS; ENERGY; HERTZSPRUNG-RUSSELL DIAGRAM; STAR EVOLUTION; STARS
- Descriptors DEC
- DIAGRAMS; EQUATIONS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent