Transport processes and chemical evolution in steady accretion disk flows

Astronomy and Astrophysics

Volumn 415, Issue 2, 2004, Pages 643-659

  Ilgner, M ^a   Henning, Th ^b   Markwick, A J ^c   Millar, T J ^c  

^a UNIVERSITY OF TÜBINGEN   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF MANCHESTER   (United Kingdom)

Author keywords

ISM: abundances; ISM: evolution; ISM: molecules; Protoplanetary disks; Solar system: formation; Stars: circumstellar matter

Indexed keywords

ASTRONOMY; CALCULATIONS; DIFFUSION; GALAXIES; HYDRODYNAMICS; KINETIC THEORY; MASS TRANSFER; MOLECULES; SOLAR SYSTEM; SPACE RESEARCH; SULFUR; TRANSPORT PROPERTIES;

CHEMICAL EVOLUTION; PROTOPLANETRY ACCRETION DISK; STARS; STEADY ACCRETION DISK FLOWS; SULPHUR BEARING MOLECULES;

PLANETS;

EID: 1442285294     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034061     Document Type: Article

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