XTE J1829-098 Predicted for Another Outburst in Early April

Details XTE J1829-098 Predicted for Another Outburst in Early April XTE J1829-098 Predicted for Another Outburst in Early April

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2007....1m&link_type=abstract

The Astronomer's Telegram, #2007

Astronomy and Astrophysics

Astronomy

Infra-Red, X-Ray, Request For Observations, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

XTE J1829-098 is a 7.8 second transient X-ray pulsar discovered by RXTE in 2004 (ATEL #317), having XMM, Chandra, and IR counterparts (Halpern & Gotthelf 2007, ApJ, 669, 579). A long term light curve of XTE J1829-098 from regular RXTE PCA monitoring observations shows that its outbursts have a recurrence period of ~246 days and a duration of ~7 days. Based on our earlier prediction, RXTE caught an outburst of the source in August 2008, appearing to peak around 2008-08-04.

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