Modeling the NIR-silhouette massive disk candidate in M 17

Astronomy and Astrophysics

Volumn 456, Issue 3, 2006, Pages 1013-1026

  Steinacker, J ^a,b   Chini, R ^c   Nielbock, M ^c   Nurnberger D ^d   Hoffmeister, V ^c   Hure J M ^e,f,g   Semenov, D ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b ASTRONOMISCHES RECHEN INSTITUT   (Germany)

^c RUHR UNIVERSITY BOCHUM   (Germany)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^e OBSERVATOIRE DE BORDEAUX   (France)

^f UNIVERSITÉ DE BORDEAUX   (France)

^g OBSERVATOIRE DE PARIS   (France)

Author keywords

Accretion, accretion disks; Radiative transfer; Stars: circumstellar matter; Stars: formation

Indexed keywords

DUST; GAS DYNAMICS; GRAVITATIONAL EFFECTS; IMAGE PROCESSING; LIGHT SCATTERING; POLYCYCLIC AROMATIC HYDROCARBONS; RADIATORS;

ACCRETION DISKS; RADIATIVE TRANSFER; STARS: CIRCUMSTELLAR MATTER; STARS: FORMATION;

ASTROPHYSICS;

EID: 33748934186     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054312     Document Type: Article

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