Very Extended X-ray and H-alpha Emission in M82: Implications for the Superwind Phenomenon
We discuss the properties and implications of a 3.7x0.9 kpc region of spatially-coincident X-ray and H-alpha emission about 11.6 kpc to the north of the galaxy M82 previously discussed by Devine and Bally (1999). The PSPC X-ray spectrum is fit by thermal plasma (kT=0.80+-0.17 keV) absorbed by only t...
Main Authors: | , , |
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Format: | Text |
Language: | unknown |
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arXiv
1999
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Online Access: | https://dx.doi.org/10.48550/arxiv.astro-ph/9904227 https://arxiv.org/abs/astro-ph/9904227 |