The VMC survey: III. Mass-loss rates and luminosities of LMC AGB stars

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Gullieuszik, M ^a   Groenewegen, M A T ^a   L Cioni, M R ^b,c   De Grijs, R ^d,e   Van Loon, J Th ^f   Girardi, L ^g   Ivanov, V D ^h   Oliveira, J M ^f   Emerson, J P ⁱ   Guandalini, R ^b  

^a ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^b UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^c UNIVERSITY OF MUNICH   (Germany)

^d PEKING UNIVERSITY   (China)

^e Kyung Hee University   (South Korea)

^f KEELE UNIVERSITY   (United Kingdom)

^g INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^h EUROPEAN SOUTHERN OBSERVATORY   (Chile)

ⁱ QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

Author keywords

Magellanic Clouds; stars: AGB and post AGB; stars: mass loss

Indexed keywords

AGB STARS; ASYMPTOTIC GIANT BRANCH STARS; BOLOMETRIC LUMINOSITIES; CHEMICAL CLASSIFICATION; CLASSIFICATION TECHNIQUE; DIRECT MEASURES; EVOLUTIONARY MODELS; EXPLORATORY STUDIES; INTERSTELLAR MEDIUMS; LARGE MAGELLANIC CLOUDS; LITERATURE DATA; MAGELLANIC CLOUDS; MASS LOSS RATE; MASS-LOSS; MIDINFRARED; RADIATIVE TRANSFER MODEL; SMALL AREA; SPECTRAL ENERGY DISTRIBUTION; STARS: AGB AND POST-AGB; STARS: MASS-LOSS; STELLAR EVOLUTIONS; STELLAR POPULATIONS; THEORETICAL MODELS;

C (PROGRAMMING LANGUAGE); CLOUDS; DUST; GALAXIES; LUMINANCE; RADIATIVE TRANSFER; SPECTROSCOPY; SURVEYS;

STARS;

EID: 84855969026     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117493     Document Type: Article

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