610 citations · 1.6k across the 17 of their papers we have counts for
17 papers
Carbon, Helium and Proton Kinetic Temperatures in a Cygnus Loop Shock Wave
J. C. Raymond, R. J. Edgar, P. Ghavamian +1
Observations of SN1006 have shown that ions and electrons in the plasma behind fast supernova remnant shock waves are far from equilibrium, with the electron temperature much lower…
Resolving the Origin of the Diffuse Soft X-ray Background
Randall K. Smith, Adam R. Foster, Richard J. Edgar +1
The ubiquitous diffuse soft (1/4 keV) X-ray background was one of the earliest discoveries of X-ray astronomy. At least some of the emission may arise from charge exchange between…
The Chandra ACIS Survey of M33 (ChASeM33): The final source catalog
R. Tuellmann, T. J. Gaetz, P. P. Plucinsky +16
This study presents the final source catalog of the Chandra ACIS Survey of M33 (ChASeM33). With a total exposure time of 1.4 Ms, ChASeM33 covers ~70% of the D25 isophote (R\approx4…
Shock Speed, Cosmic Ray Pressure, and Gas Temperature in the Cygnus Loop
Greg Salvesen, John C. Raymond, Richard J. Edgar
Upper limits on the shock speeds in supernova remnants can be combined with post-shock temperatures to obtain upper limits on the ratio of cosmic ray to gas pressure (P_CR / P_G) b…
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…
Chandra ACIS Survey of M33 (ChASeM33): X-ray Imaging Spectroscopy of M33SNR21, the Brightest X-ray Supernova Remnant in M33
Terrance J. Gaetz, William P. Blair, John P. Hughes +11
We present and interpret new X-ray data for M33SNR21, the brightest X-ray supernova remnant (SNR) in M33. The SNR is in seen projection against (and appears to be interacting with)…