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19992011
most citedX-ray Spectral Study of the Photoionized Stellar Wind in Vela~X-1

156 citations · 777 across the 25 of their papers we have counts for

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Showing 2003Show all

8 papers · 1 filter

astro-ph2003

Chandra Phase-Resolved Spectroscopy of the Crab Pulsar

Martin C. Weisskopf, Stephen L. O'Dell, Frits Paerels +3

We present the first phase-resolved study of the X-ray spectral properties of the Crab Pulsar that covers all pulse phases. The superb angular resolution of the Chandra X-ray Obser…

astro-ph20031 cited

High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models

John R. Peterson, Steven M. Kahn, Frits B. S. Paerels +5

We present XMM-Newton Reflection Grating Spectrometer observations of X-ray clusters and groups of galaxies. We demonstrate the failure of the standard cooling-flow model to descri…

astro-ph2003

Spatially resolved X-ray spectroscopy of cooling clusters of galaxies

J. S. Kaastra, T. Tamura, J. R. Peterson +7

We present spatially resolved X-ray spectra taken with the EPIC cameras of XMM-Newton of a sample of 17 cooling clusters and three non-cooling clusters for comparison. The deprojec…

astro-ph20035 cited

Structure and Dynamics of Stellar Winds in High-mass X-ray Binaries

M. Sako, S. M. Kahn, F. Paerels +4

A review of spectroscopic results obtained from Chandra High Energy Transmission Grating Spectrometer and XMM-Newton Reflection Grating Spectrometer observations of several wind-fe…

astro-ph2003

Detection of a Fully-resolved Compton Shoulder of the Iron K-alpha Line in the Chandra X-ray Spectrum of GX 301-2

Shin Watanabe, Masao Sako, Manabu Ishida +7

We report the detection of a fully-resolved, Compton-scattered emission line in the X-ray spectrum of the massive binary GX 301-2 obtained with the High Energy Transmission Grating…

astro-ph2003

XMM-Newton observations of the Vela pulsar

Kaya Mori, Charles J. Hailey, Frits Paerels +1

We present spectral analysis from XMM-Newton observations of the Vela pulsar. We analyzed thermal emission from the pulsar dominating below ~ 1 keV since extracted spectra are heav…