activity
19982009
most citedDiscovery of a flux-related change of the cyclotron line energy in Her X-1

180 citations · 1k across the 17 of their papers we have counts for

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Showing 2005Show all

10 papers · 1 filter

astro-ph2005

INTEGRAL and RXTE Observations of Centaurus A

Richard E. Rothschild, Joern Wilms, John Tomsick +6

INTEGRAL and RXTE performed three simultaneous observations of the nearby radio galaxy Cen A in 2003 March, 2004 January, and 2004 February with the goals of investigating the geom…

astro-ph2005

The Galactic black hole transient H1743-322 during outburst decay: connections between timing noise, state transitions and radio emission

E. Kalemci, J. A. Tomsick, R. E. Rothschild +3

Multi-wavelength observations of Galactic black hole transients during outburst decay are instrumental for our understanding of the accretion geometry and the formation of outflows…

astro-ph2005

3A 0535+262 in outburst

P. Kretschmar, K. Pottschmidt, C. Ferrigno +10

The Be/X-ray binary 3A 0535+262 has the highest magnetic field determined by cyclotron line studies of all accreting X-ray pulsars, despite an open debate if the fundamental line w…

astro-ph2005

RXTE Discovery of Multiple Cyclotron Lines during the 2004 December Outburst of V0332+53

K. Pottschmidt, I. Kreykenbohm, J. Wilms +6

We present an analysis of the 2-150 keV spectrum of the transient X-ray pulsar V0332+53 taken with the Rossi X-Ray Timing Explorer (RXTE) in 2004 December. We report on the detecti…

astro-ph2005

Observation of V0332+53 over the 2004/2005 outburst with Integral

I. Kreykenbohm, N. Mowlavi, K. Pottschmidt +8

We present the spectral and temporal analysis of the 2004/2005 outburst of the transient X-ray pulsar V0332+53 as observed with Integral. After the discovery of the third cyclotron…

astro-ph2005

Chandra and RXTE Spectra of the Burster GS 1826-238

T. W. J. Thompson, R. E. Rothschild, J. A. Tomsick +1

Using simultaneous observations from Chandra and RXTE, we investigated the LMXB GS 1826-238 with the goal of studying its spectral and timing properties. The uninterrupted Chandra…