The complex structure of the disk around HD 100546: The inner few astronomical units

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Benisty, M ^a   Tatulli, E ^b   Menard F ^b   Swain, M R ^c  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Accretion, Accretion disks; Instrumentation: interferometers; Radiative transfer

Indexed keywords

ACCRETION , ACCRETION DISKS; ANISOTROPIC SCATTERING; ASTRONOMICAL UNITS; BAND EMISSION; BE STARS; BEST MODEL; CIRCUMSTELLAR DISKS; CLOSE DISTANCE; COMPLEX STRUCTURE; DISK GEOMETRIES; DISK MODEL; DISK STRUCTURES; DUST GRAINS; EJECTION PROCESS; FAR INFRARED; HERBIG AEBE; HOT DUST; INSTRUMENTATION: INTERFEROMETERS; INTENSE RADIATION FIELD; INTERFEROMETRIC DATA; LARGE-GRAIN; MIDINFRARED; MONTE CARLO; NEAR INFRARED; PLANET FORMATION; SMALL GRAINS; SUBLIMATION TEMPERATURE; SURFACE LAYERS; THERMAL EMISSIONS; VERTICAL STRUCTURES;

INFRARED DEVICES; INSTRUMENTS; INTERFEROMETERS; INTERFEROMETRY; RADIATIVE TRANSFER; SILICATES; STARS; THREE DIMENSIONAL;

DUST;

EID: 79952854695     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913590     Document Type: Article

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