Galactic Superwind: Cold versus Hot Model

Details Galactic Superwind: Cold versus Hot Model Galactic Superwind: Cold versus Hot Model

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..308s&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astrophysics

Galaxies: Ism, Galaxies: Starburst, Hydrodynamics

Scientific paper

Here I reanalyze the well-known steady-state supergalactic wind solution. I show that superwinds driven by compact and powerful starbursts undergo a catastrophic cooling close to the star cluster surface and establish temperature distributions that are radically different from the adiabatic solution. The observational implications of the cold wind model both in @x X-ray and visible line regimes are discussed.

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