3D continuum radiative transfer in complex dust configurations II. 3D structure of the dense molecular cloud core ρ Oph D

Astronomy and Astrophysics

Volumn 434, Issue 1, 2005, Pages 167-180

  Steinacker, J ^a   Bacmann, A ^b,c   Henning, Th ^a   Klessen, R ^d   Stickel, M ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c OBSERVATOIRE DE BORDEAUX   (France)

^d ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Infrared: stars; ISM: dust, extinction; Methods: numerical; Radiative transfer; Stars: circumstellar mater; Stars: formation

Indexed keywords

ANNEALING; CLOUDS; COMPUTER SIMULATION; CONDENSATION; DUST; IMAGE ANALYSIS; KINEMATICS; OPTIMIZATION; SPACE TELESCOPES;

INFRARED: STARS; ISM: DUST, EXTINCTION; METHODS: NUMERICAL; RADIATIVE TRANSFER; STARS: CIRCUMSTELLAR MATER; STARS: FORMATION;

ASTROPHYSICS;

EID: 17444396288     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041978     Document Type: Article

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