Observations of millisecond X-ray pulsars
Abstract
I present an observational review of the five accretion-driven millisecond X-ray pulsars currently known, focusing on the results obtained with the Rossi X-ray Timing Explorer (RXTE) satellite. A prominent place in this review is given to the first such system discovered, SAX J1808.4-3658. Currently four outbursts have been detected from this source, three of which have been studied using RXTE. This makes this source the best studied example of all accretion-driven millisecond pulsars. Its October 2002 outburst is of particular interest because of the discovery of kilohertz quasi-periodic oscillations and burst oscillations during its thermonuclear X-ray bursts. The other four accreting millisecond pulsars were discovered within the last two years and only limited results have been published so far. A more extended review can be found at http://zon.wins.uva.nl/~rudy/admxp/
Cite
@article{arxiv.astro-ph/0403409,
title = {Observations of millisecond X-ray pulsars},
author = {Rudy Wijnands},
journal= {arXiv preprint arXiv:astro-ph/0403409},
year = {2009}
}
Comments
To appear in the proceedings of "X-ray Timing 2003: Rossi and Beyond", eds. P. Kaaret, F. K. Lamb, & J. H. Swank (Melvill, NY; AIP). A more extended version of this review can be found at http://zon.wins.uva.nl/~rudy/admxp/