NASA NTRS · 20040005900
X-ray Emission in the Large Magellanic Cloud
Abstract
All HRI images of the LMC was mosaicked. The HRI mosaic has been presented in various meetings. We have identified point and diffuse X-ray sources and analyzing their X-ray properties. The HRI mosaic has been included in papers studying individual interstellar features as well as large-scale distribution of hot gas. The results have been published in several papers.
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Chu, You-Hua, Snowden, Steve, Gruendl, Robert, Points, Sean. 2003-09-09. X-ray Emission in the Large Magellanic Cloud. https://ntrs.nasa.gov/citations/20040005900
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