Wind from a starburst galaxy nucleus

Details Wind from a starburst galaxy nucleus Wind from a starburst galaxy nucleus

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.317...44c&link_type=abstract

Nature (ISSN 0028-0836), vol. 317, Sept. 5, 1985, p. 44, 45.

Astronomy and Astrophysics

Astronomy

379

Galactic Nuclei, Starburst Galaxies, Stellar Winds, Supernovae, Astronomical Models, Galactic Radiation, Gas Pressure, X Ray Sources

Scientific paper

Galaxies with highly active star formation regions (starburst galaxies) are inferred to have high supernova rates in the region of activity. If most of the supernova energy input is thermalized, a strong wind is driven out of the active region. The authors present an analytical solution for the wind which is driven from a region of uniform mass and energy deposition. The solution is applied to M82 - the best observed case of a starburst galaxy.

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