High Frequency Quasi-Periodic Oscillations in the X-ray Flux of the Black Hole Candidate H 1743-322 = IGR/XTE J1746(4)-3213

Details High Frequency Quasi-Periodic Oscillations in the X-ray Flux of the Black Hole Candidate H 1743-322 = IGR/XTE J1746(4)-3213 High Frequency Quasi-Periodic Oscillations in the X-ray Flux of the Black Hole Candidate H 1743-322 = IGR/XTE J1746(4)-3213

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..162....1h&link_type=abstract

The Astronomer's Telegram, #162

Astronomy and Astrophysics

Astronomy

20

Radio, Far-Infra-Red, Infra-Red, Optical, X-Ray, Binaries, Black Holes, Transients

Scientific paper

We report on a ~25 ks RXTE observation of the soft X-ray transient and black hole candidate H 1743-322 (= IGR/XTE J1746(4)-3213, see ATELs 146, 142, 141, 140, 139, 138, 137, 136, 133, 132) performed on May 28 2003 (05:02 UTC - 16:53 UTC). The source was observed at a 3-100 keV flux of ~2.5x10e-8 ergs/cm^2/s with a spectrum that could be fitted well with a disk black body (kT~1.2 keV) and a power law (index~2.6) extending to above 200 keV with no apparent cutoff.

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