Wind-driven gas networks and star formation in galaxies: Reaction-advection hydrodynamic simulations

Monthly Notices of the Royal Astronomical Society

Volumn 325, Issue 1, 2001, Pages 1-33

  Chappell, David ^a,b   Scalo, John ^a  

^a UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^b UNIVERSITY OF LA VERNE   (United States)

Author keywords

Galaxies: ISM; Hydrodynamics; ISM: bubbles; Stars: formation; Turbulence

Indexed keywords

ADVECTION; CONTINUUM MECHANICS; HYDRODYNAMICS; KINETIC ENERGY; KINETICS; MASS SPECTROMETERS; MASS SPECTROMETRY; MASS TRANSFER; MORPHOLOGY; SOLVENTS; STARS; VELOCITY; VELOCITY DISTRIBUTION;

COLUMN DENSITY; EXPONENTIAL TAIL; GALAXIES: ISM; GAS NETWORKS; GAS VELOCITY; GRAVITATIONAL INSTABILITY; ISM: BUBBLE; STAR CLUSTERS; STAR FORMATION RATES; STARS FORMATION;

GASES;

EID: 0007802257     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04196.x     Document Type: Article

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