1.9k citations · 4.7k across the 71 of their papers we have counts for
8 papers · 2 filters
Relations Between Timing Features and Colors in Accreting Millisecond Pulsars
Steve van Straaten, Michiel van der Klis, Rudy Wijnands
We have studied the aperiodic X-ray timing and color behavior of the accreting millisecond pulsars SAX J1808.4-3658, XTE J1751-305, XTE J0929-314, and XTE J1814-338 using large dat…
X-ray variability during the quiescent state of the neutron-star X-ray transient in the globular cluster NGC 6440
Edward M. Cackett, Rudy Wijnands, Craig O. Heinke +6
The globular cluster NGC 6440 is known to harbor a bright neutron-star X-ray transient. We observed the globular cluster with Chandra on two occasions when the bright transient was…
High- and low-frequency quasi-periodic oscillations in the X-ray light curves of the black hole transient H1743-322
Jeroen Homan, Jon M. Miller, Rudy Wijnands +4
We present a variability study of the black hole candidate and X-ray transient H1743-322 during its 2003/2004 outburst. We analyzed five Rossi X-ray Timing Explorer observations th…
Simultaneous Chandra and RXTE Spectroscopy of the Microquasar H~1743-322: Clues to Disk Wind and Jet Formation from a Variable Ionized Outflow
J. M. Miller, J. Raymond, J. Homan +7
We observed the bright phase of the 2003 outburst of the Galactic black hole candidate H 1743-322 in X-rays simultaneously with Chandra and RXTE on four occasions. The Chandra/HETG…
Chandra observations of the accretion-driven millisecond X-ray pulsars XTE J0929-314 and XTE J1751-305 in quiescence
Rudy Wijnands, Jeroen Homan, Craig O. Heinke +2
(Abridge) We observed the accreting millisecond X-ray pulsars XTE J0929-314 and XTE J1751-305 in their quiescent states using Chandra. From XTE J0929-314 we detected 22 photons (0.…
Crust cooling curves of accretion-heated neutron stars
Rudy Wijnands
We discuss the recent efforts to use a sub-class of neutron-star X-ray transients (the quasi-persistent transients) to probe the properties of neutron-star crusts and cores. Quasi-…