Physical and radiative properties of the first-core accretion shock

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Commercon B ^a,b,c   Audit, E ^b   Chabrier, G ^c,d   Chieze J P ^b  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITÉ DE LYON   (France)

^d UNIVERSITY OF EXETER   (United Kingdom)

Author keywords

Hydrodynamics; Methods: analytical; Methods: numerical; Radiative transfer; Stars: formation

Indexed keywords

HYDRODYNAMICS; NUMERICAL METHODS; RADIATIVE TRANSFER; SHOCK WAVES; STARS;

BAROTROPIC APPROXIMATIONS; CHARACTERISTIC PROPERTIES; DIFFUSION APPROXIMATIONS; METHODS: NUMERICALS; METHODS:ANALYTICAL; RADIATION HYDRODYNAMICS; STAR-FORMATION PROCESS; STARS: FORMATION;

ANALYTICAL MODELS;

EID: 79955418864     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016213     Document Type: Article

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