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The M82 Outflow: X-rays as a Probe for Neutral Disk Gas

Published online by Cambridge University Press:  26 May 2016

Jürgen Ott ,
Fabian Walter  and
Jürgen Kerp
Jürgen Ott
Affiliation:
ATNF, CSIRO, Marsfield NSW 2122, Australia
Fabian Walter
Affiliation:
NRAO-AOC, P.O. Box O, Socorro, NM 87801, USA
Jürgen Kerp
Affiliation:
RAIUB, Auf dem Hügel 71, 53121 Bonn, Germany

Abstract

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We present an analysis of X-ray absorption in the nearby starburst galaxy M82. The X-ray attenuating column densities in the northern part of the M 82 outflow can be associated with cold disk gas detected in maps of H1 and CO (1→0). We derive an XCO factor which is somewhat lower as compared to that in our Galaxy. This is in good agreement with multi-transition line studies of various molecules in the disk of M 82.

Type
Part 3. Ejection and Outflow
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 312 - 313
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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