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20002008
most citedM 33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary

62 citations · 206 across the 6 of their papers we have counts for

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astro-ph200817 cited

XMM-Newton observations of the Small Magellanic Cloud: XMMU J004814.1-731003, a 25.55 s Be/X-ray binary pulsar

F. Haberl, P. Eger, W. Pietsch +2

To investigate candidates for Be/X-ray binaries in the Small Magellanic Cloud (SMC), we observed a region around the emission nebula N19 with XMM-Newton in October 2006. We analyse…

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-ph200635 cited

Evidence for Shocked Molecular Gas in the Galactic SNR CTB 109 (G109.1-1.0)

Manami Sasaki, Roland Kothes, Paul P. Plucinsky +2

We report the detection of molecular clouds around the X-ray bright interior feature in the Galactic supernova remnant (SNR) CTB 109 (G109.1-1.0). This feature, called the Lobe, ha…

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…

astro-ph200625 cited

FUV and X-ray Observations of the Reverse Shock in the SMC SNR 1E 0102.2-7219

Manami Sasaki, Terrance J. Gaetz, William B. Blair +4

We present FUSE and XMM-Newton data for the reverse shock of the O-rich SNR 1E0102.2-7219 in the SMC. The FUSE observations cover three regions with significantly different optical…