Synthetic photometry for carbon rich giants I. Hydrostatic dust-free models

Astronomy and Astrophysics

Volumn 503, Issue 3, 2009, Pages 913-928

  Aringer, B ^a,b,c   Girardi, L ^b   Nowotny, W ^a   Marigo, P ^c   Lederer, M T ^a  

^a UNIVERSITY OF VIENNA   (Austria)

^b INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^c UNIVERSITY OF PADOVA   (Italy)

Author keywords

Hertzsprung Russell (HR) and C M diagrams; Infrared stars; Stars AGB and post AGB; Stars atmospheres; Stars carbon; Stars late type

Indexed keywords

CARBON RICH; CARBON STARS; CIRCUMSTELLAR; CIRCUMSTELLAR DUST; COMMONLY USED; DYNAMICAL PHENOMENA; EFFECTIVE TEMPERATURE; FILTER SYSTEM; FREE MODEL; FUNDAMENTAL PARAMETERS; HERTZSPRUNG-RUSSELL AND C-M DIAGRAMS; HYDROSTATIC MODEL; INFRARED LIGHT; INFRARED STARS; LATE STAGE; LOW AND INTERMEDIATE MASS STARS; LOW RESOLUTION; MASS LOSS; MASS LOSS RATE; MEASURED DATA; METALLICITIES; PHOTOMETRIC DATA; PHOTOMETRIC PROPERTIES; POPULATION SYNTHESIS; STARS ATMOSPHERES; STELLAR EVOLUTIONS; STELLAR PARAMETERS; STRUCTURAL CHANGE; SURFACE GRAVITY; SYNTHETIC PHOTOMETRY;

ATMOSPHERIC TEMPERATURE; BIOLOGY; DUST; HYDRAULICS; HYDRODYNAMICS; PHOTOMETRY;

STARS;

EID: 77149146592     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911703     Document Type: Article

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