Characterizing the velocity field in hydrodynamical simulations of low-mass star formation using spectral line profiles

Astronomy and Astrophysics

Volumn 489, Issue 2, 2008, Pages 607-616

  Brinch, C ^a   Hogerheijde, M R ^a   Richling, S ^b  

^a LEIDEN UNIVERSITY   (Netherlands)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

Hydrodynamics; ISM: molecules; Line: profiles; Radiative transfer; Stars: formation

Indexed keywords

DESIGN; DIFFRACTIVE OPTICAL ELEMENTS; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); EMISSION SPECTROSCOPY; ROTATING DISKS; SPECTRUM ANALYSIS;

CLOUD MORPHOLOGY; DYNAMICAL BEHAVIORS; DYNAMICAL STRUCTURES; HYDRODYNAMICAL MODELS; HYDRODYNAMICS; INITIAL CONDITIONS; INTERFEROMETRIC DATA; ISM: MOLECULES; KNOW-HOW; LINE EXCITATION; LINE: PROFILES; LOW-MASS STAR FORMATION; LOW-MASS STARS; PARAMETERIZED; PARAMETERIZED MODELING; PROTO-PLANETARY DISKS; RADIATION TRANSFER; RADIATIVE TRANSFER; SIMPLE MODELING; SPECTRAL EMISSIONS; SPECTRAL ENERGY DISTRIBUTIONS; SPECTRAL LINE PROFILES; STARS: FORMATION; SUB-MILLIMETER; VELOCITY FIELDS; YOUNG STELLAR OBJECTS;

CURVE FITTING;

EID: 52949109246     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810034     Document Type: Article

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