Published March 1973
| Version v1
Journal article
X-ray emission from white dwarfs in close binary systems
Description
The generation of X-ray sources in close binary systems is studied. It is proposed that one of the stars is a white dwarf and it is accreting material from its companion. The entire treatment applies to the sphericaly symmetric and the stationary case. The model of this type accounts qualitatively for the observed nature of SCO X-1.
Additional details
Identifiers
- DOI
- 10.1143/ptp.49.776;
Publishing Information
- Journal Title
- Progress of Theoretical Physics
- Journal Volume
- 49
- Journal Issue
- 3
- Series
- Progr. Theor. Phys. (Kyoto).
- Journal Page Range
- 776-789
- ISSN
- 0033-068X
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 4086969
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; BREMSSTRAHLUNG; COSMIC X-RAY SOURCES; HARD X RADIATION; HOT PLASMA; IMPLOSIONS; SHOCK WAVES; STAR EVOLUTION; STEADY FLOW; SUPERSONIC FLOW; ULTRAHIGH TEMPERATURE; WHITE DWARF STARS
- Descriptors DEC
- DWARF STARS; ELECTROMAGNETIC RADIATION; FLUID FLOW; PLASMA; RADIATIONS; STARS; X RADIATION
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent