Spin down rate and inferred dipole magnetic field of the new soft gamma-ray repeater SGR 1833-0832

Details Spin down rate and inferred dipole magnetic field of the new soft gamma-ray repeater SGR 1833-0832 Spin down rate and inferred dipole magnetic field of the new soft gamma-ray repeater SGR 1833-0832

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2550....1e&link_type=abstract

The Astronomer's Telegram, #2550

Astronomy and Astrophysics

Astronomy

2

X-Ray, Pulsars, Soft Gamma-Ray Repeaters

Scientific paper

We observed the new soft gamma-ray repeater SGR 1833-0832 with XMM-Newton on 2010 March 23 (for about 22 ks) and on 2010 April 02 (for about 21 ks). By merging these data sets with those collected since the discovery of the source (GCN #10526) with RossiXTE and Swift, we were able to refine the period measurement reported in ATEL #2494 (see also ATEL #2493), also including in the phase-coherent timing solution a first period derivative component.

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