Identification of galactic bulge X ray bursts with persistent X ray counterparts

Details Identification of galactic bulge X ray bursts with persistent X ray counterparts Identification of galactic bulge X ray bursts with persistent X ray counterparts

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..567p&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 567-572 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

2

Galactic Bulge, Radio Bursts, X Ray Astronomy, X Ray Sources, X Ray Spectra, Imaging Spectrometers, Mir Space Station, Spaceborne Astronomy, X Ray Telescopes

Scientific paper

Details of five X ray bursts seen during a survey of the galactic bulge are presented. They were made with the coded-mask imaging X ray spectrometer between Oct. 1988 and Apr. 1989. The bursts are shown to originate from the previously known burst sources 1702-429, 1728-337 and from close to SLX1744-299. The results which showed that there are in fact two adjacent sources, SLX1744-299 and SLX1744-300, and that it is the latter which is a burst source, are confirmed.

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