Published 1973
| Version v1
Journal article
UHURU results on galactic x-ray sources
Creators
Description
Galactic X-ray sources studied by UHURU can be classified into several categories, including supernova remnants, transient or nova-like sources, Sco X-1 like sources, and pulsating sources. The latter are discussed in some detail with particular emphasis upon the characteristics of the periodic binary X-ray sources, Cen X-3 and Her X-1. It is suggested that all galactic X-ray sources (except S/N remnants) may be binary systems.
Additional details
Identifiers
Publishing Information
- Journal Title
- Symposium - International Astronomical Union
- Journal Volume
- 55
- Journal Issue
- no.55
- Series
- Int. Astron. Union Symp.
- Journal Page Range
- 9-28
- ISSN
- 0074-1809
Conference
- Title
- Symposium X - and gamma-ray astronomy.
- Dates
- 11 May 1972.
- Place
- Madrid, Spain.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 5108430
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; MILKY WAY; PULSES; SATELLITES; SUPERNOVA REMNANTS
- Descriptors DEC
- COSMIC RADIO SOURCES; GALAXIES; STARS
Optional Information
- Notes
- See CONF-720599--.; Updated automatically by Metadata and Full-Text Enrichment Agent