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19932011
most citedThe evolution of the timing properties of the black-hole transient GX 339-4 during its 2002/2003 outburst

499 citations · 3.8k across the 60 of their papers we have counts for

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astro-ph2005★ 25 cited

A Chandra X-ray observation of the globular cluster Terzan 1

E. M. Cackett, R. Wijnands, C. O. Heinke +6

We present a 19 ks Chandra ACIS-S observation of the globular cluster Terzan 1. Fourteen sources are detected within 1.4 arcmin of the cluster center with 2 of these sources predic…

astro-ph2005★ 57 cited

XMM-Newton observations of the black hole X-ray transient XTE J1650-500 in quiescence

Jeroen Homan, Rudy Wijnands, Albert Kong +4

We report the result of an XMM-Newton observation of the black-hole X-ray transient XTE J1650-500 in quiescence. The source was not detected and we set upper limits on the 0.5-10 k…

astro-ph2005

The Iron K-shell features of MXB 1728-34 from a Simultaneous Chandra-RXTE Observation

A. D' Ai, T. Di Salvo, R. Iaria +7

We report on a simultaneous Chandra and RossiXTE observation of the low-mass X-ray binary atoll bursting source MXB 1728-34 performed on 2002 March 3-5. We fit the 1.2-35 keV conti…

astro-ph2005★ 499 cited

The evolution of the timing properties of the black-hole transient GX 339-4 during its 2002/2003 outburst

T. Belloni, J. Homan, P. Casella +5

We present the results of the timing and color analysis of more than two hundred RXTE/PCA observations of the bright black-hole transient GX 339-4 obtained during its 2002/2003 out…

astro-ph2005★ 32 cited

Late-time X-Ray, UV and Optical Monitoring of Supernova 1979C

Stefan Immler, Robert A. Fesen, Schuyler D. Van Dyk +8

We present results from observations of SN 1979C with XMM-Newton in X-rays and in the UV, archival X-ray and HST data, and follow-up ground-based optical imaging. The XMM-Newton MO…

astro-ph2005

X-ray sources in globular clusters of other galaxies

Walter H. G. Lewin, Frank Verbunt

A large number of X-ray sources in globular clusters of galaxies other than the Milky Way has been found with Chandra. We discuss three issues relating to these sources. The X-ray…