most citedThe behavior of subluminous X-ray transients near the Galactic center as observed using the X-ray telescope aboard Swift

88 citations · 333 across the 7 of their papers we have counts for

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astro-ph200845 cited

Chandra and Swift observations of the quasi-persistent neutron star transient EXO 0748-676 back to quiescence

N. Degenaar, R. Wijnands, M. T. Wolff +8

The quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 recently started the transition to quiescence following an accretion outburst that lasted more t…

astro-ph20088 cited

Chandra and XMM-Newton observations of the low-luminosity X-ray pulsators SAX J1324.4-6200 and SAX J1452.8-5949

Ramanpreet Kaur, Rudy Wijnands, Alessandro Patruno +5

We present results from our Chandra and XMM-Newton observations of two low-luminosity X-ray pulsators SAX J1324.4-6200 and SAX J1452.8-5949 which have spin-periods of 172 s and 437…

astro-ph20082 cited

A New Class of Radio Pulsars - Back in 1982

M. Ali Alpar

Basic ideas about the torques on the neutron star and the existence of an equilibrium rotation period followed from the recognition that most X-ray binaries contain accretion power…

astro-ph200822 cited

The Swift capture of a long X-ray burst from XTE J1701-407

Manuel Linares, Anna L. Watts, Rudy Wijnands +5

XTE J1701-407 is a new transient X-ray source discovered on June 8th, 2008. More than one month later it showed a rare type of thermonuclear explosion: a long type I X-ray burst. W…

astro-ph200888 cited

The behavior of subluminous X-ray transients near the Galactic center as observed using the X-ray telescope aboard Swift

N. Degenaar, R. Wijnands

In this paper we report on the spectral analysis of seven X-ray transients, which were found to be active during a monitoring campaign of the Galactic center carried out in 2006 an…

astro-ph200880 cited

Cooling of the crust in the neutron star low-mass X-ray binary MXB 1659-29

Edward M. Cackett, Rudy Wijnands, Jon M. Miller +2

In quasi-persistent neutron star transients, long outbursts cause the neutron star crust to be heated out of thermal equilibrium with the rest of the star. During quiescence, the c…