Positions and evidence for a steady component for X-ray burst sources

Details Positions and evidence for a steady component for X-ray burst sources Positions and evidence for a steady component for X-ray burst sources

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976natur.262..473q&link_type=abstract

Nature, vol. 262, Aug. 5, 1976, p. 473, 474. Research supported by the Scientific Research Council.

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Spaceborne Astronomy, X Ray Astronomy, X Ray Sources, Ariel Satellites, Periodic Variations, Position (Location), Radiant Flux Density, Sas-3, Uhuru Satellite

Scientific paper

X-ray fluxes from two sources within the error boxes for burst sources MXB1730-335 and MXB1728-34 were observed in direct observations of the galactic center region in the Ariel V RMC experiment. Data referable to the positions of the events are analyzed statistically and correlated with known objects. Bursts reported earlier in association with the objects are compared. The observed flux is accepted as the integral of bursts of the type reported for the first source, while flux from the second source is attributed to non-burst background emission. The possibility that sources 3U1727-33 and MXB1728-34 may be identical, with a periodicity indicative of a slow rotator, is considered.

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