On the nature of pre-main sequence candidate stars in the Large Magellanic Cloud

Astronomy and Astrophysics

Volumn 432, Issue 2, 2005, Pages 619-632

  De Wit, W J ^a,g   Beaulieu, J P ^b   Lamers, H J G L M ^c,d   Coutures, C ^e   Meeus, G ^f  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c UTRECHT UNIVERSITY   (Netherlands)

^d SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^e DIF   (France)

^f ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^g LABORATOIRE D ASTROPHYSIQUE   (France)

Author keywords

Galaxies: Magellanic clouds; Stars: emission line, Be; Stars: formation; Stars: pre main sequence; Stars: variables: general

Indexed keywords

BE-STARS; EMISSION-LINE; PRE-MAIN SEQUENCE; STARS:FORMATION-STARS; VARIABLES;

CLOUDS; DUST; IONIZATION; METAL INSULATOR BOUNDARIES; PHOTOMETRY; REFLECTION;

GALAXIES;

EID: 15244355023     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041248     Document Type: Article

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