activity
20052020
most citedThe population of X-ray supernova remnants in the Large Magellanic Cloud

139 citations · 348 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2020★ 1 cited

Mineralogy of a Sulfate-rich Inverted Channel in the Atacama Desert, Chile: Clues to its Formation and Preservation

E. Z. Noe Dobrea, R. M. E. Williams, W. E. Dietrich +3

We have performed a stratigraphic and mineralogical analysis of a vertical transect across a ridge located at the distal end of a system of eroded alluvial deposits in the northern…

astro-ph.HE2015★ 139 cited

The population of X-ray supernova remnants in the Large Magellanic Cloud

P. Maggi, F. Haberl, P. J. Kavanagh +11

We present a comprehensive X-ray study of the population of supernova remnants (SNRs) in the LMC. Using primarily XMM-Newton, we conduct a systematic spectral analysis of LMC SNRs…

astro-ph.HE2014★ 8 cited

Physical Nature of the [S II]-Bright Shell Nebulae N70 and N185

Ning-Xiao Zhang, You-Hua Chu, R. M. Williams +3

N70 and N185 are two large (100 pc in diameter) shell nebulae in the Large Magellanic Cloud (LMC). Their high [\ion{S}{2}]/H ratios rival those of supernova remnants (SNRs)…

astro-ph.HE2012★ 30 cited

DEM L241, a Supernova Remnant containing a High-Mass X-ray Binary

F. D. Seward, P. A. Charles, D. L. Foster +5

A Chandra observation of the Large Magellanic Cloud supernova remnant DEM L241 reveals an interior unresolved source which is probably an accretion-powered binary. The optical coun…

astro-ph.CO2011★ 18 cited

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…

astro-ph.HE2009★ 23 cited

Nonthermal X-ray Emission from the N11 Superbubble in the Large Magellanic Cloud

L. A. Maddox, R. M. Williams, B. C. Dunne +1

We present the results of X-ray spectral analysis of the superbubble around the OB association LH9 in the H II complex N11 in the Large Magellanic Cloud. Using observations from Su…