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A Chandra study of the morphological structure of the Wolf-Rayet dwarf starburst galaxy NGC 4214
Published online by Cambridge University Press: 26 May 2016
Abstract
We present results from a Chandra X-ray observation of the dwarf starburst galaxy NGC 4214, a galaxy containing several young star forming regions. Starburst regions are known to be associated with diffuse X-ray emission, and in this case X-ray emission from the galaxy shows an interesting morphological structure with a bright X-ray ring of emission within the galaxy.
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- Part 4. Feedback from Massive Stars
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- Copyright © Astronomical Society of the Pacific 2003