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...
Published in: | The Astrophysical Journal |
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Main Authors: | , , |
Language: | English |
Published: |
1999
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Subjects: | |
Online Access: | https://doi.org/10.1086/307762 http://cds.cern.ch/record/384970 |