Dust-driven winds and mass loss of C-rich AGB stars with subsolar metallicities

Astronomy and Astrophysics

Volumn 486, Issue 2, 2008, Pages 497-504

  Wachter, A ^a,b   Winters, J M ^c   Schroder K P ^d   Sedlmayr, E ^a  

^a TECHNISCHE UNIVERSITÄT BERLIN   (Germany)

^b UPPSALA UNIVERSITY   (Sweden)

^c IRAM   (France)

^d UNIVERSITY OF GUANAJUATO   (Mexico)

Author keywords

Hydrodynamics; Stars: AGB and post AGB; Stars: carbon; Stars: evolution; Stars: mass loss; Stars: winds, outflows

Indexed keywords

ASTRONOMY; ASTROPHYSICS; DUST; LUMINANCE; OPTICAL PROPERTIES; STARS;

ABUNDANCE RATIOS; ASYMPTOTIC GIANT BRANCH (AGB) STARS; DUST FORMATION; DYNAMICAL MODELING; MASS LOSS RATE (MLR); MASS LOSSES; MASS STARS; METALLICITIES; METALLICITY; MODEL ASSUMPTIONS; ORDER-OF MAGNITUDES; OUTFLOW VELOCITIES; QUANTITATIVE DESCRIPTION; SECOND-MOMENT CLOSURE (SMC) MODELS; STELLAR EVOLUTIONS; STELLAR MASSES; WIND MODELING;

METALLIZING;

EID: 47249112964     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809893     Document Type: Article

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