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...

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Bibliographic Details
Main Authors: Lehnert, M. D., Heckman, T. M., Weaver, K. A.
Format: Text
Language:unknown
Published: arXiv 1999
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/9904227
https://arxiv.org/abs/astro-ph/9904227