Radiation thermo-chemical models of protoplanetary disks: I. Hydrostatic disk structure and inner rim

Astronomy and Astrophysics

Volumn 501, Issue 1, 2009, Pages 383-406

  Woitke, P ^a,b   Kamp, I ^c   F Thi, W ^d  

^a UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c UNIVERSITY OF GRONINGEN   (Netherlands)

^d UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

Astrochemistry; Methods: Numerical; Radiative transfer; Stars: Circumstellar matter; Stars: Formation

Indexed keywords

ASTROCHEMISTRY; ATOMIC GAS; CONVERTING LINES; COOLING PROCESS; DISK MODEL; DISK STRUCTURES; DUST GRAINS; EMISSION LINES; FREQUENCY-DEPENDENT; GAS ENERGY; GASPHASE; HEATING AND COOLING RATES; HERSCHEL; HIGH-DENSITY; ICE FORMATIONS; INTERSTELLAR CLOUDS; IRRADIATED SURFACE; METHODS: NUMERICAL; NON-LTE; OPTICAL LINES; PHOTO-CHEMISTRY; PROTOPLANETARY DISKS; RADIATIVE PROCESS; STARS: CIRCUMSTELLAR MATTER; STARS: FORMATION; STELLAR ATMOSPHERES; THERMOCHEMICAL MODELS; VIBRATIONAL LINES;

COOLING; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; ELECTROMAGNETIC WAVE EMISSION; GAS EMISSIONS; HEATING; HYDRAULICS; HYDRODYNAMICS; LEAKAGE (FLUID); MODELS; NUMERICAL METHODS; RADIATIVE TRANSFER; STARS; TWO DIMENSIONAL;

DENSITY OF GASES;

EID: 67650909544     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911821     Document Type: Article

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