Chandra ACIS Survey of M33 (ChASeM33): The enigmatic X-ray emission from IC131 (2009)
Tuellmann, R., Long, K. S., Pannuti, T. G., Winkler, P. F., Gaetz, T. J., Plucinsky, P. P., ...
We present the first X-ray analysis of the diffuse hot ionized gas and the point sources in IC131, after NGC604 the second most X-ray luminous giant HII region in M33. The X-ray emission is detected...
Detection of the second eclipsing high mass X-ray binary in M 33 (2008)
Pietsch, W., Haberl, F., Gaetz, T. J., Hartman, J. D., Plucinsky, P. P., Tüllmann, R., ...
Chandra data of the X-ray source [PMH2004] 47 were obtained in the ACIS Survey of M 33 (ChASeM33) in 2006. During one of the observations, the source varied from a high state to a low state and back,...
The Chandra ACIS Survey of M33 (ChASeM33): Investigating the Hot Ionized Medium in NGC604 (2008)
Tuellmann, R., Gaetz, T. J., Plucinsky, P. P., Long, K. L., Hughes, J. P., Blair, W. P., ...
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 interact with the...
M 33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary (2006)
Pietsch, W., Haberl, F., Sasaki, M., Gaetz, T. J., Plucinsky, P. P., Ghavamian, P., ...
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 and have resolved...
M33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary (2006)
Pietsch, W., Haberl, F., Sasaki, M., Gaetz, T. J., Plucinsky, P. P., Ghavamian, P., ...
Detection of the second eclipsing XRB in M33 by Chandra (2006)
Pietsch, W., Plucinsky, P. P., Haberl, F., Shporer, A., Mazeh, T.
Warren, J. S., Hughes, J. P., Badenes, C., Ghavamian, P., McKee, C. F., Moffett, D., ...
We present evidence for cosmic ray acceleration at the forward shock in Tycho's supernova remnant (SNR) from three X-ray observables: (1) the proximity of the contact discontinuity to the forward...
Chandra Observations of MBM12 and Models of the Local Bubble (2005)
Smith, R. K., Edgar, R. J., Plucinsky, P. P., Wargelin, B. J., Freeman, P. E., Biller, B. A.
Chandra observations toward the nearby molecular cloud MBM12 show unexpectedly strong and nearly equal foreground O VIII and O VII emission. As the observed portion of MBM12 is optically thick at...
XMM-Newton observations of the Galactic Supernova Remnant CTB 109 (G109.1-1.0) (2004)
Sasaki, M., Plucinsky, P. P., Gaetz, T. J., Smith, R. K., Edgar, R. J., Slane, P. O.
We present the analysis of the X-ray Multi-Mirror Mission (XMM-Newton) European Photon Imaging Camera (EPIC) data of the Galactic supernova remnant (SNR) CTB 109 (G109.1-1.0). CTB 109 is associated...
A High-Resolution Study of Nonthermal Radio and X-Ray Emission from SNR G347.3-0.5 (2003)
Lazendic, J. S., Slane, P. O., Gaensler, B. M., Reynolds, S. P., Plucinsky, P. P., Hughes, J. P.
G347.3-0.5 is one of three shell-type supernova remnants in the Galaxy whose X-ray spectrum is dominated by nonthermal emission. This puts G347.3-0.5 in the small, but growing class of SNRs for which...
Chandra Spectra of the Soft X-ray Diffuse Background (2002)
Markevitch, M., Bautz, M. W., Biller, B., Butt, Y., Edgar, R., Gaetz, T., ...
We present an exploratory Chandra ACIS-S3 study of the diffuse component of the Cosmic X-ray Background in the 0.3-7 keV band for four directions at high Galactic latitudes, with emphasis on details...
Chandra Observations of the Eastern Limb of the Vela Supernova Remnant (2001)
Plucinsky, P. P., Smith, R. K, Edgar, R. J., Gaetz, T. J., Slane, P. O., Blair, W. P., ...
We present results from two Chandra/ACIS observations of the so-called Vela ``Bullet D'' region on the eastern limb of the Vela supernova remnant. The Bullet D region is a bright X-ray feature,...
Nonthermal X-Ray Emission from G266.2-1.2 (RX J0852.0-4622) (2001)
Slane, P., Hughes, J. P., Edgar, R. J., Plucinsky, P. P., Miyata, E., Aschenbach, B.
The newly discovered supernova remnant G266.2-1.2 (RX J0852.0-4622), along the line of sight to the Vela SNR, was observed with ASCA for 120 ks. We find that the X-ray spectrum is featureless, and...