4U 1626-67 Torque Reversal Simultaneous with Swift/BAT Flux Increase

Details 4U 1626-67 Torque Reversal Simultaneous with Swift/BAT Flux Increase 4U 1626-67 Torque Reversal Simultaneous with Swift/BAT Flux Increase

Jun 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2099....1c&link_type=abstract

The Astronomer's Telegram, #2099

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

The recent torque reversal in the accretion-powered pulsar 4U 1626-67 (ATel #2095), which occurred after 18 years of steady spin-down, was centered near MJD 54500 (2008 Feb 4) and lasted about 150 days. This was simultaneous with an increase of flux reported by Krimm et al. (ATel #1426). We observed the spin-up first in the Fermi/GBM data (see our web page). Using Swift/BAT observations from 2004 up to the present, we have resolved the frequency history of this source through the torque reversal (Camero-Arranz et al.

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