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Volumn 669, Issue 2, 2007, Pages 1262-1278

Molecular line radiative transfer in protoplanetary disks: Monte Carlo simulations versus approximate methods

Author keywords

Astrochemistry; Line: formation; Line: profiles; Planetary systems: protoplanetary disks; Radiative transfer; Radio lines: stars; Stars: formation

Indexed keywords


EID: 39049129664     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/521872     Document Type: Article
Times cited : (60)

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