Published September 1977
| Version v1
Journal article
On the mass-radius relation in close binary systems
Description
In a close binary system with circular orbits in which mass transfer occurs when material from one star fills up and possibly spills over its Roche lobe, the usual mass-radius relation cannot be used as it would lead to unreasonable results in some situations. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00642455;
Publishing Information
- Journal Title
- Astrophysics and Space Science
- Journal Volume
- 51
- Journal Issue
- 1
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 33-38
- ISSN
- 0004-640X
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 9366680
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; MASS TRANSFER; ORBITAL ANGULAR MOMENTUM; ROCHE EQUIPOTENTIALS
- Descriptors DEC
- ANGULAR MOMENTUM; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent