SIGMA/GRANAT observations of hard X-ray emission from type I X-ray bursters

Details SIGMA/GRANAT observations of hard X-ray emission from type I X-ray bursters SIGMA/GRANAT observations of hard X-ray emission from type I X-ray bursters

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..719b&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 12, p. (12)719-(12)722

Astronomy and Astrophysics

Astronomy

1

Accretion Disks, Binary Stars, Bursts, Globular Clusters, Neutron Stars, Stellar Magnetic Fields, X Ray Astronomy, X Rays, Astronomical Catalogs, Black Holes (Astronomy), Heao 2, Rosat Mission, Satellite-Borne Instruments, X Ray Telescopes

Scientific paper

Unlike black hole candidate systems, accreting neutron stars seem to encounter appreciable difficulties in emitting strong hard X-ray fluxes. However, in the catalog of the hard X-ray sources detected by SIGMA, three sources are associated with type I X-ray bursters. In this paper, we review the present status of the SIGMA observations of these three X-ray burst sources, namely X 1724-308 in the globular cluster Terzan II, KS 1731-260, and GX 354+0.

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