R
R. M. Williams
Researcher at Columbus State University
Publications - 13
Citations - 382
R. M. Williams is an academic researcher from Columbus State University. The author has contributed to research in topics: Large Magellanic Cloud & Galaxy. The author has an hindex of 10, co-authored 13 publications receiving 328 citations.
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Journal ArticleDOI
The population of X-ray supernova remnants in the Large Magellanic Cloud
P. Maggi,Frank Haberl,P. J. Kavanagh,Manami Sasaki,Luke M Bozzetto,Miroslav Filipovic,Georgios Vasilopoulos,Wolfgang Pietsch,Sean D Points,You-Hua Chu,John R. Dickel,Matthias Ehle,R. M. Williams,Jochen Greiner +13 more
TL;DR: In this article, a comprehensive X-ray study of the population of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) using primarily XMM-Newton observations was conducted to gain new insight into their evolution and the interplay with their host galaxy.
Journal ArticleDOI
The population of X-ray supernova remnants in the Large Magellanic Cloud
P. Maggi,Frank Haberl,P. J. Kavanagh,Manami Sasaki,Luke M Bozzetto,Miroslav Filipovic,Georgios Vasilopoulos,Wolfgang Pietsch,Sean D Points,You-Hua Chu,John R. Dickel,Matthias Ehle,R. M. Williams,Jochen Greiner +13 more
TL;DR: In this paper, a comprehensive X-ray study of the population of supernova remnants (SNRs) in the Local Group (LMC) is presented, which provides a complete census of LMC SNRs exhibiting Fe K lines.
Journal ArticleDOI
DEM L241, a Supernova Remnant containing a High-Mass X-ray Binary
F. D. Seward,P. A. Charles,P. A. Charles,Deatrick Foster,John R. Dickel,P. S. Romero,Zachary I. Edwards,M. R. Perry,R. M. Williams +8 more
TL;DR: In this paper, Chandra observations of the Large Magellanic Cloud supernova remnant DEM L241 reveal an interior unresolved source which is probably an accretion-powered binary with an orbital period of tens of days.
Journal ArticleDOI
Nonthermal X-ray Emission from the N11 Superbubble in the Large Magellanic Cloud
TL;DR: In this article, the authors 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.
Journal ArticleDOI
Nonthermal x-ray emission in the n11 superbubble in the large magellanic cloud
TL;DR: In this paper, the authors present the results of X-ray spectral analysis of the superbubble (SB) around the OB association LH9 in the H II complex N11 in the Large Magellanic Cloud.