Swift/XRT monitoring of the long outburst of the Very Faint X-ray Transient XMMU J174716.1-281048

Details Swift/XRT monitoring of the long outburst of the Very Faint X-ray Transient XMMU J174716.1-281048 Swift/XRT monitoring of the long outburst of the Very Faint X-ray Transient XMMU J174716.1-281048

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2624....1d&link_type=abstract

The Astronomer's Telegram, #2624

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Transients

Scientific paper

The Very Faint X-ray Transient (VFXT) XMMU J174716.1-281048, discovered in 2003 by XMM-Newton (ATel #147 and Sidoli et al., 2006, A&A 456, 287), is a type I burster (ATel #970; #972; Del Santo et al., 2007, A&A 468, L17) lying in the Galactic Centre region (ATel #1207). XMMU J174716.1-281048 is the first source classified as ``quasi persistent" VFXT, because it is in outburst since 2003 (Del Santo et al., 2007, A&A 468, L17; ATel #1078).

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