Published September 1977
| Version v1
Journal article
Sco X-1
Creators
- 1. Tokyo Univ. (Japan). Inst. of Space and Aeronautical Science
Description
The physical properties of X-ray, optical and radio emissions from Sco X-1 are reviewed. Sco X-1 is a typical X-ray source which has an optically thick hot plasma. The observational spectra of X-ray and optical emissions are consistent with theoretical ones from the hot plasma, but the radio emission shows a non-thermal feature. The restrictive conditions for the model of Sco X-1 are discussed from the observational facts. In spite of numerous observational facts on Sco X-1 further detailed and elaborate studies are necessary to understand this object and general compact X-ray sources comprehensively. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf02431834;
Publishing Information
- Journal Title
- Space Science Reviews
- Journal Volume
- 20
- Journal Issue
- 6
- Series
- Space Sci. Rev.
- Journal Page Range
- 687-755
- ISSN
- 0038-6308
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 9361719
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; EMISSION SPECTRA; HARD X RADIATION; HOT PLASMA; OPTICALLY THICK PLASMA; PHOTOMETRY; POLARIZATION; RADIOWAVE RADIATION; RED DWARF STARS; SOFT X RADIATION; STAR MODELS; VARIATIONS; VISIBLE RADIATION; X-RAY SPECTRA
- Descriptors DEC
- COSMIC RAY SOURCES; DWARF STARS; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MATHEMATICAL MODELS; PLASMA; RADIATIONS; SPECTRA; STARS; X RADIATION
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent