The mass-loss return from evolved stars to the Large Magellanic Cloud: V. the GRAMS carbon-star model grid

Astronomy and Astrophysics

Volumn 532, Issue , 2011, Pages

  Srinivasan, S ^a   Sargent, B A ^b   Meixner, M ^b  

^a INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^b STScI   (United States)

Author keywords

Circumstellar matter; Magellanic Clouds; Radiative transfer; Stars: AGB and post AGB; Stars: carbon; Stars: mass loss

Indexed keywords

CIRCUMSTELLAR MATTERS; MAGELLANIC CLOUDS; STARS: CARBON; STARS: MASS-LOSS; STARS:AGB AND POST AGB;

AMORPHOUS CARBON; AMORPHOUS SILICON; DUST; GALAXIES; GRAIN SIZE AND SHAPE; INFRARED DEVICES; LUMINANCE; PHOTOMETERS; PHOTOMETRY; RADIATION; RADIATIVE TRANSFER; SHELLS (STRUCTURES); SILICON CARBIDE; SPECTROSCOPY; SURVEYS;

STARS;

EID: 79960629934     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117033     Document Type: Article

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