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20022008
most citedThe Dearth of low-luminosity Globular Cluster LMXBs in NGC 3379

3 citations · 5 across the 6 of their papers we have counts for

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astro-ph2007

X-ray supernova remnants in nearby galaxies

Ioanna Leonidaki, Andreas Zezas, Panayotis Boumis

We present the initial results from a study of the SNR population in a sample of six nearby galaxies (NGC 2403, NGC 4214, NGC 4449, NGC 5204, NGC 3077, NGC 4395) based on Chandra a…

astro-ph200744 cited

Deep Chandra Monitoring Observations of NGC 3379: Catalog of Source Properties

N. J. Brassington, G. Fabbiano, D. -W. Kim +11

We present the properties of the discrete X-ray sources detected in our monitoring program of the `typical' elliptical galaxy, NGC 3379, observed with Chandra ACIS-S in five separa…

astro-ph20073 cited

The Dearth of low-luminosity Globular Cluster LMXBs in NGC 3379

G. Fabbiano, N. J. Brassington, A. Zezas +10

Our campaign of deep monitoring observations with {\it Chandra} of the nearby elliptical galaxy NGC 3379 has lead to the detection of nine globular cluster (GC) and 53 field low ma…

astro-ph2007141 cited

The Orbital Period of the Wolf-Rayet Binary IC 10 X-1; Dynamic Evidence that the Compact Object is a Black Hole

A. H. Prestwich, R. Kilgard, P. A. Crowther +6

IC 10 X-1 is a bright (Lx=10^38 ergs/s) variable X-ray source in the local group starburst galaxy IC 10. The most plausible optical counterpart is a luminous Wolf-Rayet star, makin…

astro-ph200713 cited

The X-ray binary population in M33: II. X-ray spectra and variability

H. -J. Grimm, J. McDowell, A. Zezas +2

In this paper we investigate the X-ray spectra and X-ray spectral variability of compact X-ray sources for 3 Chandra observations of the Local Group galaxy M33. The observations ar…

astro-ph2007249 cited

Occultation measurement of the size of the X-ray emitting region in the Active Galactic Nucleus of NGC 1365

G. Risaliti, M. Elvis, G. Fabbiano +3

We present an occultation of the central X-ray emitting region in the Seyfert Galaxy NGC 1365. This extreme spectral variation (from Compton-thin to reflection-dominated and back t…