Radiation thermo-chemical models of protoplanetary disks. II. Line diagnostics

Astronomy and Astrophysics

Volumn 510, Issue 1, 2010, Pages

  Kamp, I ^a   Tilling, I ^b   Woitke, P ^b   Thi, W F ^b   Hogerheijde, M ^c  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^c LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Astrochemistry; Circumstellar matter; Line: formation; Methods: numerical; Radiative transfer; Stars: formation

Indexed keywords

ASTROCHEMISTRY; ATOMIC SURFACES; CHEMICAL ABUNDANCE; CIRCUMSTELLAR MATTERS; CRITICAL DENSITY; DISK MODEL; FINE STRUCTURES; FORMATION PROCESS; GAS MASS; HERSCHEL; HOT REGIONS; LINE PROFILES; LINE: FORMATION; LOW-MASS; M-LINES; MASS INDICATOR; MONTE CARLO; MULTIPARAMETERS; NON-LTE; PEAK SEPARATIONS; PHYSICO-CHEMICALS; PROTOPLANETARY DISKS; RADIATIVE TRANSFER - STARS; RADIATIVE TRANSFER CODES; SURFACE AREA; SURFACE LAYERS; THERMOCHEMICAL MODELS; TOTAL EMISSIONS;

DISKS (MACHINE COMPONENTS); NUMERICAL METHODS; RADIATIVE TRANSFER; STARS;

DISKS (STRUCTURAL COMPONENTS);

EID: 77149153049     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913076     Document Type: Article

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