Discovery of an X-ray pulsar in the low-mass X-ray binary 2A 1822-371
Abstract
We report the discovery of 0.59 s X-ray pulsations from the low-mass X-ray binary, 5.57 hr dipping and eclipsing ADC source 2A 1822-371. Pulse arrival time analysis indicates a circular orbit with e < 0.03 (95% confidence) and an asini for the neutron star of 1.006(5) lightseconds, implying a mass function of (2.03+-0.03) x 10^-2 M_sun. The barycentric pulse period was 0.59325(2) s in 1996.270 and 0.59308615(5) s in 1998.205, indicating an average spin up with P_dot/P = (-1.52+-0.02) x 10^-4 yr^-1. For a magnetic field strength of ~1--5 x 10^12 G as derived from the X-ray spectrum the implied intrinsic X-ray luminosity is ~2-4 x 10^37 erg s^-1. The pulse amplitude is low, but increases steeply as a function of energy from a sinusoidal amplitude of 0.25% in 2-5.4 keV to ~3% above 20 keV. We discuss the constraints on the masses of the companion star and the fact that several aspects of the energy spectrum are in qualitative accordance with that of a strongly magnetised neutron star.
Cite
@article{arxiv.astro-ph/0104356,
title = {Discovery of an X-ray pulsar in the low-mass X-ray binary 2A 1822-371},
author = {Peter G. Jonker and Michiel van der Klis},
journal= {arXiv preprint arXiv:astro-ph/0104356},
year = {2009}
}
Comments
6 pages long, including 4 figures, uses emulateapj5, accepted for ApJL, Replaced figure 1