RXTE Observations of the hard galactic bulge source SLX 1735-269

Details RXTE Observations of the hard galactic bulge source SLX 1735-269 RXTE Observations of the hard galactic bulge source SLX 1735-269

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.361s&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Since its discovery during the 1985 Spacelab-2 flight, SLX 1735-269 has been found to be one of the persistent emitters of high energy X-rays in the galactic bulge. Observation with SAX of an X-ray burst has recently shown that this system contains a neutron star, contrary to some early speculation. We report here on the analysis of spectral and temporal data obtained during a 50 ksec RXTE observation of this source undertaken to further elucidate the nature of this object.

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