First determination of the dynamical mass of a binary L dwarf

Astronomy and Astrophysics

Volumn 423, Issue 1, 2004, Pages 341-352

  Bouy, H ^a,b,d   Duchene G ^d,f   Kohler R ^c   Brandner, W ^c   Bouvier, J ^d   Martin E L ^e   Ghez, A ^f   Delfosse, X ^d   Forveille, T ^d,j   Allard, F ^g   Baraffe, I ^g   Basri, G ^h   Close, L ⁱ   McCabe, C E ^f  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^d LABORATOIRE D ASTROPHYSIQUE   (France)

^e INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITÉ DE LYON   (France)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF ARIZONA   (United States)

^j CANADA FRANCE HAWAII TELESCOPE   (United States)

more..

Author keywords

Star: individual: 2MASSW J0746425+2000321; Stars: binaries: visual; Stars: binary (including multiple): close; Stars: low mass, brown dwarfs; Techniques: high angular resolution

Indexed keywords

APPROXIMATION THEORY; IMAGE ANALYSIS; MASS SPECTROMETRY; OBSERVATORIES; PHOTOMETRY; PHYSICAL PROPERTIES; TELESCOPES; TEMPERATURE CONTROL;

BINARIES; BROWN DWARF-STARS; CLOSE-TECHNIQUE; HIGH ANGULAR RESOLUTION-STARS; LOW-MASS; STARS; VISUAL;

ASTRONOMY;

EID: 4043093584     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040551     Document Type: Article

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