On the spin-down rate of Swift J1822.3-1606

Details On the spin-down rate of Swift J1822.3-1606 On the spin-down rate of Swift J1822.3-1606

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3944....1i&link_type=abstract

The Astronomer's Telegram, #3944

Astronomy and Astrophysics

Astronomy

X-Ray, Neutron Star, Soft Gamma-Ray Repeater, Transient, Variables, Pulsar

Scientific paper

After more than 7.5 months since the burst detection from Swift
J1822.3-1606 (occurred on 2011 July the 14th; Cummings et al. ATel.
#3488) more than 60 pointings have been collected.

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