UHURU results on galactic x-ray sources
Conference
·
· Int. Astron. Union Symp., no. 55, pp. 9-28
OSTI ID:4426720
From symposium X-and gamma-ray astronomy; Madrid, Spain (11 May 1972). See CONF-720599-. Galactic x-ray sources studied by Uhuru can be claasified 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. (auth)
- Research Organization:
- American Science and Engineering, Cambridge, MA
- NSA Number:
- NSA-29-008488
- OSTI ID:
- 4426720
- Journal Information:
- Int. Astron. Union Symp., no. 55, pp. 9-28, Journal Name: Int. Astron. Union Symp., no. 55, pp. 9-28; ISSN IAUSA
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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