The density variance-mach number relation in the taurus molecular cloud

Astronomy and Astrophysics

Volumn 513, Issue 12, 2010, Pages

  Brunt, C M ^a  

^a UNIVERSITY OF EXETER   (United Kingdom)

Author keywords

ISM: kinematics and dynamics; ISM: molecules; Magnetohydrodynamics (MHD); Radio lines: ISM; Techniques: spectroscopic; Turbulence

Indexed keywords

AERODYNAMICS; CLOUDS; DUST; HIGH FREQUENCY TELECOMMUNICATION LINES; KINEMATICS; MACH NUMBER; PHOTOMAPPING; POWER SPECTRUM; RADIO WAVES; SPECTROSCOPY; TURBULENCE;

ANALYTIC MODELS; COLUMN DENSITY; COMPRESSIVE MODE; DENSITY ENHANCEMENT; DENSITY FLUCTUATION; ESTIMATED PARAMETER; ISM: KINEMATICS AND DYNAMICS; ISM: MOLECULES; LOW COLUMN DENSITY; MOLECULAR CLOUDS; NUMERICAL MODELS; POWER-SPECTRA; RADIO LINES: ISM; SPATIAL DIFFERENCES; SPECTRAL LINE; STAR FORMATIONS; SUBRESOLUTION; SUPERSONIC TURBULENCE;

MAGNETOHYDRODYNAMICS;

EID: 77951827189     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913506     Document Type: Article

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