Lyman-α emission properties of simulated galaxies: Interstellar medium structure and inclination effects

Astronomy and Astrophysics

Volumn 546, Issue , 2012, Pages

  Verhamme, A ^a,b,c,d   Dubois, Y ^a,e   Blaizot, J ^b,c,d   Garel, T ^b,c,d,f   Bacon, R ^b   Devriendt, J ^a,b,c,d   Guiderdoni, B ^b,c,d   Slyz, A ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b UNIVERSITÉ DE LYON   (France)

^c UNIVERSITÉ LYON 1   (France)

^d CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^e INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^f SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

Author keywords

Galaxies: ISM; Hydrodynamics; ISM: kinematics and dynamics; ISM: structure; Methods: numerical; Radiative transfer

Indexed keywords

CONTINUUM RADIATION; DARK MATTER HALOS; DOUBLE PEAK; EMISSION PROPERTIES; EQUIVALENT WIDTH; GALAXIES: ISM; GALAXY FORMATIONS; GALAXY SIMULATIONS; GIANT MOLECULAR CLOUDS; HYDRODYNAMICS SIMULATIONS; INTERNAL ENERGIES; INTERSTELLAR MEDIUMS; ISM: KINEMATICS AND DYNAMICS; ISM: STRUCTURE; LINE OF SIGHT; METAL LINE; METHODS: NUMERICALS; NARROW BANDS; NUMERICAL RESOLUTION; RADIATION TRANSFER; RED-SHIFTED; SELECTION FUNCTION; STRINGENT REQUIREMENT; STRUCTURATION; VELOCITY FIELD; YOUNG STARS;

HYDRODYNAMICS; NUMERICAL METHODS; PHOTONS; RADIATION EFFECTS; RADIATIVE TRANSFER; STARS; SURVEYS; VELOCITY;

GALAXIES;

EID: 84867635916     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201218783     Document Type: Article

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