Re-brightening of XMMSL1 J171900.4-353217

Details Re-brightening of XMMSL1 J171900.4-353217 Re-brightening of XMMSL1 J171900.4-353217

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2722....1a&link_type=abstract

The Astronomer's Telegram, #2722

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Black Holes, Neutron Stars, Transients

Scientific paper

We continued our Swift-XRT monitoring of the new very-faint X-ray source XMMSL1 J171900.4-353217 [ATel #2607, #2656]. Two new observations were obtained on Jun 14th and 29th and we fitted both observations with an absorbed powerlaw model, keeping the hydrogen column density constant to the value 3.4E22 cm-2 (see ATel #2627). The resulting photon index is 2.16+/-0.28 and 2.11+/-0.14 respectively and the absorbed (unabsorbed) flux in 2-10 keV range is 1.67E-11 (2.3E-11) ergs cm-2 s-1 and 5.12E-11 (7E-11) respectively.

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