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astro-ph200819 cited

The Chandra ACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium in NGC604

R. Tuellmann, T. J. Gaetz, P. P. Plucinsky +7

NGC604 is the largest HII-region in M33, second only within the Local Group to 30 Dor, and is important as a laboratory for understanding how massive young stellar clusters interac…

astro-ph200817 cited

The Chandra ACIS Survey of M33 (ChASeM33): Transient X-ray Sources Discovered in M33

Benjamin F. Williams, Terrance J. Gaetz, Frank Haberl +7

The Chandra ACIS Survey of M33 (ChASeM33) has acquired 7 fields of ACIS data covering M33 with 200 ks of exposure in each field. A catalog from the first 10 months of data, along w…

astro-ph200750 cited

Chandra ACIS Survey of M33 (ChASeM33): A First Look

Paul P. Plucinsky, Benjamin Williams, Knox S. Long +22

We present an overview of the Chandra ACIS Survey of M33 (ChASeM33): A Deep Survey of the Nearest Face-on Spiral Galaxy. The 1.4 Ms survey covers the galaxy out to $R \approx 18\ar…

astro-ph200719 cited

A Statistical Study of Galactic SNRs using the PMN Survey

M. Stupar, M. D. Filipovic, Q. A. Parker +3

The Parkes-MIT-NRAO (PMN) radio survey has been used to generate a quasi all-sky study of Galactic Supernova Remnants (SNRs) at a common frequency of 4.85 GHz. We present flux dens…

astro-ph200616 cited

An Analysis of the Broadband (22-3900 MHz) Radio Spectrum of HB3 (G132.7+1.3): The Detection of Thermal Radio Emission from an Evolved Supernova Remnant?

D. Urosevic, T. Pannuti, D. Leahy

We present an analysis of the broadband radio spectrum (from 22 to 3900 MHz) of the Galactic supernova remnant (SNR) HB3 (G132.7+1.3). Published observations have revealed that a c…

astro-ph200662 cited

M 33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary

W. Pietsch, F. Haberl, M. Sasaki +5

The first observations conducted as part of the Chandra ACIS survey of M 33 (ChASeM33) sampled the eclipsing X-ray binary M 33 X-7 over a large part of the 3.45 d orbital period an…