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Simple Model of the Outflow from Starburst Galaxies: Application to Radio Observations

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© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation V. N. Zirakashvili and H. J. Völk 2006 ApJ 636 140 DOI 10.1086/497900

0004-637X/636/1/140

Abstract

We present an analytical model for the hydrodynamic outflow from the disk of a starburst galaxy. The model is used to calculate the cosmic-ray propagation and the radio intensity distribution in the nuclear starburst region of NGC 253. We find that the cosmic-ray energy production rate of the central 600 pc of NGC 253 is about 3 × 1041 ergs s-1, which is about 15% of the total mechanical supernova power. For this inner region, we estimate a terminal outflow velocity of 900 km s-1 and a mass-loss rate of = 2-4 M yr-1.

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10.1086/497900