SiO in C-rich circumstellar envelopes of AGB stars: Effects of non-LTE chemistry and grain adsorption

Astronomy and Astrophysics

Volumn 454, Issue 1, 2006, Pages 247-255

  Schoier F L ^a   Olofsson, H ^a,b   Lundgren, A A ^c  

^a ALBANOVA UNIVERSITY CENTER   (Sweden)

^b CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

Author keywords

Stars: AGB and post AGB; Stars: carbon; Stars: circumstellar matter; Stars: late type; Stars: mass loss

Indexed keywords

ADSORPTION; ASTROPHYSICS; CARBON; COMPUTER SIMULATION; DUST; GRAIN GROWTH; PARTICULATE EMISSIONS;

RADIATIVE TRANSFER MODELING; SIO ABUNDANCE DISTRIBUTION; STARS: AGB AND POST-AGB; STARS: CARBON; STARS: CIRCUMSTELLAR MATTER; STARS: LATE-TYPE; STARS: MASS-LOSS;

SILICON COMPOUNDS;

EID: 33746450384     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054795     Document Type: Article

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