Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3576....1g&link_type=abstract
The Astronomer's Telegram, #3576
Astronomy and Astrophysics
Astronomy
X-Ray, Neutron Star, Soft Gamma-Ray Repeater
Scientific paper
Swift J1834.9-0846 (D'Elia et al. GCN Circ. 12253, Guiriec et al. 12255) was observed with Chandra/ACIS-S on 2011 August 22 for a 13 ks net exposure time. The timing analysis of the barycentered data in the 0.5-8 keV range clearly reveal the coherent signal at 0.40285032 Hz that is consistent with our earlier report (Gogus et al. ATel 2542) and confirms it as the spin frequency of the new source.
Gogus Ersin
Kargaltsev Oleg
Kouveliotou Chryssa
Pavlov George G.
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