Published 1976
| Version v1
Report
''Other'' galactic x-ray sources
Description
There is by now a ''standard'' model for x-ray sources comprising a binary system containing a compact star and powered by mass accretion. It can be argued that the majority and perhaps all the galactic x-ray sources are of this kind. Three kinds of sources are discussed which may be qualitatively different from these; namely, low luminosity sources such as 3U0352 + 30 (= chi Perseus.), the sources associated with the globular clusters, and the transient x-ray sources
Additional details
Publishing Information
- Imprint Title
- X-ray binaries
- Journal Page Range
- p. 669-676.
- Report number
- CONF-7510169--
Conference
- Title
- Symposium on x-ray binaries.
- Dates
- 20 - 22 Oct 1975.
- Place
- Greenbelt, Maryland, United States of America (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 9364330
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; GALAXIES; LUMINOSITY; STAR ACCRETION; STRUCTURAL MODELS
- Descriptors DEC
- COSMIC RAY SOURCES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STAR EVOLUTION; STARS