Three-component modeling of C-rich AGB star winds. I. Method and first results

Astronomy and Astrophysics

Volumn 398, Issue 1, 2003, Pages 253-266

  Sandin, C ^a   Hofner S ^a  

^a UPPSALA UNIVERSITY   (Sweden)

Author keywords

Hydrodynamics; Instabilities; Radiative transfer; Stars: AGB and post AGB; Stars: mass loss

Indexed keywords

APPROXIMATION THEORY; ENERGY TRANSFER; EQUATIONS OF MOTION; HYDRODYNAMICS; MASS TRANSFER;

STAR WINDS;

ASTROPHYSICS;

EID: 0037250813     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021643     Document Type: Article

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