The substellar mass function in σ Orionis II. Optical, near-infrared and IRAC/Spitzer photometry of young cluster brown dwarfs and planetary-mass objects

Astronomy and Astrophysics

Volumn 470, Issue 3, 2007, Pages 903-918

  Caballero, J A ^a,b   Bejar V J S ^a   Rebolo, R ^a,c   Eisloffel J ^d   Osorio, M R Zapatero ^a,e   Mundt, R ^b   Barrado y Navascues D ^e   Bihain, G ^a,c   Bailer Jones, C A L ^b   Forveille, T ^f,g   Martin E L ^a,h  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c CSIC   (Spain)

^d Consejo Superior de Investigaciones Científicas ^*  (Germany)

^e INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL   (Spain)

^f CANADA FRANCE HAWAII TELESCOPE   (United States)

^g LABORATOIRE D ASTROPHYSIQUE   (France)

^h UNIVERSITY OF CENTRAL FLORIDA   (United States)

Author keywords

Galaxy: open clusters and associations: individual: Orionis; Stars: low mass, brown dwarfs; Stars: planetary systems: protoplanetary discs

Indexed keywords

PROTOPLANETARY DISCS; STARS: PLANETARY SYSTEMS;

ASTROPHYSICS; MASS TRANSFER; PHOTOMETRY; PLANETS;

STARS;

EID: 34547657695     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066993     Document Type: Article

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