Chemical abundances of late-type pre-main sequence stars in the σ Orionis cluster

Astronomy and Astrophysics

Volumn 490, Issue 3, 2008, Pages 1135-1142

  Gonzalez Hernandez J I ^a,b   Caballero, J A ^c,d   Rebolo, R ^d,e   Bejar V J S ^d   Barrado Y Navascues D ^f   Martin E L ^d   Zapatero Osorio, M R ^d  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b Marie Curie Excellence Team ^*  (France)

^c UNIVERSIDAD COMPLUTENSE DE MADRID   (Spain)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e CSIC   (Spain)

^f INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL   (Spain)

Author keywords

Galaxy: open clusters and associations: individual: Orionis; Stars: abundances; Stars: pre main sequence

Indexed keywords

CALCIUM; COSMOLOGY; LITHIUM; PHOTOGRAPHY; RANDOM ERRORS; SILICON; SYSTEMATIC ERRORS;

ALMOST CONSISTENT; AND SYSTEMATIC ERRORS; ATMOSPHERIC ABUNDANCES; BROWN DWARFS; CHEMICAL ABUNDANCES; CONSISTENT; EFFECTIVE TEMPERATURES; ERROR BARS; FUNDAMENTAL PARAMETERS; INFRARED; MAIN SEQUENCE STARS; METALLICITY; MODEL ATMOSPHERES; OPTICAL; OPTICAL SPECTROSCOPIES; RADIAL VELOCITIES; STARS: ABUNDANCES; STARS: PRE-MAIN SEQUENCE; STELLAR SURFACES; WILLIAM HERSCHEL TELESCOPES;

STARS;

EID: 54949097823     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810398     Document Type: Article

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