Model infrared spectra of passively heated proto-planetary disks surrounding intermediate-mass pre-main-sequence stars

Astronomy and Astrophysics

Volumn 496, Issue 3, 2009, Pages 741-749

  Meijer, J ^a   Waters, L B F M ^a,b   De Koter, A ^a,c   Min, M ^a   Van Boekel, R ^d   Dominik, C ^a,e   Dullemond, C P ^d  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b KU LEUVEN   (Belgium)

^c UTRECHT UNIVERSITY   (Netherlands)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

Author keywords

Stars: circumstellar matter; Stars: planetary systems: protoplanetary disks; Stars: pre main sequence

Indexed keywords

CRYSTALLINE SILICATES; DISK GEOMETRIES; DISK MODEL; DUST PARTICLE; FORSTERITE; HYDROSTATIC EQUILIBRIUM; INFRARED SPECTRUM; IR SPECTRUM; LONG DISTANCES; M-SPECTRUM; MIDINFRARED; MODEL PARAMETERS; PRE-MAIN-SEQUENCE; PROTOPLANETARY DISKS; SPATIAL DISTRIBUTION; SPECTRAL REGION; SPECTRAL SHAPES; STARS: CIRCUMSTELLAR MATTER; STARS: PLANETARY SYSTEMS: PROTOPLANETARY DISKS; STARS: PRE-MAIN SEQUENCE; THEORETICAL SPECTRA; VERTICAL DISTRIBUTIONS;

CRYSTALLINE MATERIALS; CRYSTALLOGRAPHY; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; EMISSION SPECTROSCOPY; LITHOLOGY; MINERALOGY; MINERALS; OLIVINE; RESONANCE; SILICATES; SIZE DISTRIBUTION; SPECTRUM ANALYSIS; STARS;

INFRARED SPECTROSCOPY;

EID: 65949123337     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200809547     Document Type: Article

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