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...

Full description

Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Lehnert, M D, Heckman, T M, Weaver, K A
Language:English
Published: 1999
Subjects:
Online Access:https://doi.org/10.1086/307762
http://cds.cern.ch/record/384970