115 citations · 601 across the 13 of their papers we have counts for
12 papers
Can Charge Exchange Explain Anomalous Soft X-ray Emission in the Cygnus Loop?
Renata S. Cumbee, David B. Henley, Phillip C. Stancil +4
Recent X-ray studies have shown that supernova shock models are unable to satisfactorily explain X-ray emission in the rim of the Cygnus Loop. In an attempt to account for this ano…
Modeling the X-rays Resulting from High Velocity Clouds
Robin L. Shelton, Kyujin Kwak, David B. Henley
With the goal of understanding why X-rays have been reported near some high velocity clouds, we perform detailed 3 dimensional hydrodynamic and magnetohydrodynamic simulations of c…
An X-ray Investigation of Three Supernova Remnants in the Large Magellanic Cloud
Matthew D. Klimek, S. D. Points, R. C. Smith +2
We have investigated three SNRs in the LMC using multi-wavelength data. These SNRs are generally fainter than the known sample and may represent a previously missed population. One…
G65.2+5.7: A Thermal Composite Supernova Remnant With a Cool Shell
R. L. Shelton, K. D. Kuntz, R. Petre
This paper presents archival ROSAT PSPC observations of the G65.2+5.7 supernova remnant (also known as G65.3+5.7). Little material obscures this remnant and so it was well observed…
Chandra Observations and Models of the Mixed-Morphology Supernova Remnant W44: Global Trends
R. L. Shelton, K. D. Kuntz, R. Petre
As with other mixed morphology remnants, W44's projected center is bright in thermal X-rays. It has an obvious radio shell, but no discernable X-ray shell. X-ray bright knots dot W…
Supernova Remnants in the Magellanic Clouds. IV. X-Ray Emission from the Largest SNR in the LMC
R. M. Williams, Y. -H. Chu, J. R. Dickel +4
We present the first X-ray detection of SNR 0450-70.9 the largest known supernova remnant (SNR) in the Large Magellanic Cloud. To study the physical conditions of this SNR, we have…