Swift/XRT monitoring of the latest outburst from XMMUJ174716.1-281048

Details Swift/XRT monitoring of the latest outburst from XMMUJ174716.1-281048 Swift/XRT monitoring of the latest outburst from XMMUJ174716.1-281048

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1174....1s&link_type=abstract

The Astronomer's Telegram, #1174

Astronomy and Astrophysics

Astronomy

5

Binaries, Transients

Scientific paper

We are performing a monitoring with Swift/XRT of the Very Faint X-ray Transient (VFXT) XMMUJ174716.1-281048 (ATel #147 and Sidoli et al., 2006, A&A 456, 287) which is undergoing an accretion phase since 2003 (Del Santo et al., 2007, A&A 468, L17; ATel #1078, #1136). To date, this is the first VFXT displaying a ``quasi persistent" behaviour. Swift/XRT observed the source four times: on 13 and 17 May 2007 (results reported by Degenaar et al.

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