Increased flux of HETE J1900.1-2455 detected with both Swift/XRT and RXTE/PCA

Details Increased flux of HETE J1900.1-2455 detected with both Swift/XRT and RXTE/PCA Increased flux of HETE J1900.1-2455 detected with both Swift/XRT and RXTE/PCA

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1106....1d&link_type=abstract

The Astronomer's Telegram, #1106

Astronomy and Astrophysics

Astronomy

5

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

Following the non-detection of HETE J1900.1-2455 on June 6 (ATel #1098), we find this system considerably brighter in a ~5 ksec Swift/XRT observation performed on June 10, 2007 (2:25-12:14 UT). The X-ray spectrum can be well described by an absorbed powerlaw plus blackbody model, with Nh~0.19, kT~0.16 keV and a photon index of ~2.24. The inferred 2.0-10.0 keV flux is ~2.8E-10 erg/cm2/s, which corresponds to an X-ray luminosity ~8.4E35 (d/5kpc) erg/s.

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