Swift/XRT monitoring of XMMU J174716.1-281048: still active!

Details Swift/XRT monitoring of XMMU J174716.1-281048: still active! Swift/XRT monitoring of XMMU J174716.1-281048: still active!

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2050....1d&link_type=abstract

The Astronomer's Telegram, #2050

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

The Very Faint X-ray Transient (VFXT) XMMU J174716.1-281048 (ATel #147 and Sidoli et al., 2006, A&A 456, 287) is being observed with Swift/XRT since May 2007 (ATel #1078), in order to monitor the level of activity during the latest outburst, which started in 2003 (Del Santo et al., 2007, A&A 468, L17; ATels #1078, #1136, #1174, #1496). XMMU J174716.1-281048 is indeed the first source classified as "quasi persistent" VFXT.

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