Re-brightening of XTE J1719-291

Details Re-brightening of XTE J1719-291 Re-brightening of XTE J1719-291

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1467....1d&link_type=abstract

The Astronomer's Telegram, #1467

Astronomy and Astrophysics

Astronomy

3

Binaries, Black Holes, Neutron Stars, Transients

Scientific paper

After our first Swift/XRT observation (ATEL #1451) of the new, very faint X-ray transient XTE J1719-291 (ATEL #1442), we acquired two additional observations to monitor the flux evolution of this source. The first additional observation was performed on April 3, 2008, and lasted ~2.6 ksec. The source was detected at a count rate which was slightly less than the previous observation (0.045 counts/s versus 0.051 counts/s).

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