New Timing Results of the X-ray Binary Pulsar OAO 1657-415

Details New Timing Results of the X-ray Binary Pulsar OAO 1657-415 New Timing Results of the X-ray Binary Pulsar OAO 1657-415

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1379..212j&link_type=abstract

ASTROPHYSICS OF NEUTRON STARS 2010: A Conference in Honor of M. Ali Alpar. AIP Conference Proceedings, Volume 1379, pp. 212-213

Astronomy and Astrophysics

Astrophysics

1

Pulsars, X-Ray Binary Stars, Gamma-Ray Sources (Astronomical), X-Rays, Pulsars, X-Ray Binaries, Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray

Scientific paper

OAO 1657-415 is an eclipsing X-ray binary pulsar that has undergone several torque reversals throughout its long history of observation. We present a frequency history spanning nearly 19 years of observations from the Burst and Transient Source Experiment (BATSE) and from the Gamma-Ray Burst Monitor (GBM). Orbital ephemerides of the pulsar system is obtained at several intervals throughout this history. With these ephemerides, statistically significant orbital decay is established.

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