Synthetic H i observations of a simulated spiral galaxy

Monthly Notices of the Royal Astronomical Society

Volumn 406, Issue 3, 2010, Pages 1460-1470

  Acreman, David M ^a   Douglas, Kevin A ^a   Dobbs, Clare L ^a,b,c   Brunt, Christopher M ^a  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF MUNICH   (Germany)

Author keywords

Galaxies: individual: M31; Galaxies: individual: M33; Methods: numerical; Radiative transfer; Radio lines: galaxies

Indexed keywords

HYDRODYNAMICS; NUMERICAL METHODS; RADIATIVE TRANSFER; RAY TRACING; VELOCITY;

ADAPTIVE MESH REFINEMENT; GALAXIES: INDIVIDUAL: M33; GALAXIES: INDIVIDUALS; GALAXY: INDIVIDUAL: M31; METHOD: NUMERICAL; RADIO LINES:GALAXIES; REFINEMENT GRIDS; SMOOTHED PARTICLE HYDRODYNAMICS; SPIRAL GALAXIES; VELOCITY CHANNELS;

GALAXIES;

EID: 77955263269     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16858.x     Document Type: Article

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