Likely New Outburst from XTE J1550-564

Details Likely New Outburst from XTE J1550-564 Likely New Outburst from XTE J1550-564

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000atel...58....1s&link_type=abstract

The Astronomer's Telegram, #58

Astronomy and Astrophysics

Astronomy

X-Ray, Request For Observations, Binaries, Black Holes, Transients

Scientific paper

Observations over 2000 April 6-10 with the RXTE All-Sky Monitor show a clear detection of a source with maximum likelihood position 1 +- 3 arcmin from the position of XTE J1550-564 (IAUC #7009). It is therefore highly likely that we have detected renewed activity of XTE J1550-564. A 2-12 keV light curve from this location shows an approximately linear flux increase at a rate of ~15+-2 mCrab/day, an order of magnitude slower than the rate of increase during the onset of the XTE J1550-564 outburst in 1998 (IAUC #7008, ATEL #37).

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