Quiescent X-ray variability from the neutron star transient Aql X-1

Authors

E. M. Cackett, Institute of Astronomy, University of CambridgeFollow
J. K. Fridriksson, MIT Kavli Institute for Astrophysics and Space Research
J. Homan, MIT Kavli Institute for Astrophysics and Space Research
J. M. Miller, University of Michigan
R. Wijnands, Astronomical Institute 'Anton Pannekoek', University of Amsterdam

Document Type

Article

Abstract

A number of studies have revealed variability from neutron star low-mass X-ray binaries during quiescence. Such variability is not well characterized, or understood, but may be a common property that has been missed due to lack of multiple observations. One such source where variability has been observed is Aql X-1. Here, we analyse 14 Chandra and XMM-Newton observations of Aql X-1 in quiescence, covering a period of approximately 2 yr. There is clear variability between the epochs, with the most striking feature being a flare-like increase in the flux by a factor of 5. Spectral fitting is inconclusive as to whether the power-law and/or thermal component is variable. We suggest that the variability and flare-like behaviour during quiescence is due to accretion at low rates which might reach the neutron star surface.

Disciplines

Cosmology, Relativity, and Gravity | Stars, Interstellar Medium and the Galaxy

Comments

NOTICE IN COMPLIANCE WITH PUBLISHER POLICY: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©2011 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society. All rights reserved. Available at doi:10.1111/j.1365-2966.2011.18601.x

Recommended Citation

Cackett, E. M., Fridriksson, J. K., Homan, J., Miller, J. M., Wijnands, R. 2011. Quiescent X-ray variability from the neutron star transient Aql X-1. MNRAS 414(4), 3006-3013.