Detection of the second period derivative in the timing evolution of SGR 1833-0832

Details Detection of the second period derivative in the timing evolution of SGR 1833-0832 Detection of the second period derivative in the timing evolution of SGR 1833-0832

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2691....1e&link_type=abstract

The Astronomer's Telegram, #2691

Astronomy and Astrophysics

Astronomy

X-Ray, Pulsars, Soft Gamma-Ray Repeaters

Scientific paper

SGR 1833-0832 was monitored with XMM-Newton, Swift, and RossiXTE since its discovery by Swift, thanks to the BAT detection of a short burst on 2010 March 19 (MJD 55274; GCN #10526). After about 90 days since the BAT event, we detect an additional component with respect to the phase-coherent timing solutions previously reported, which included only the period and its first time derivative.

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