Physical parameters of T dwarfs derived from high-resolution near-infrared spectra

Astronomy and Astrophysics

Volumn 501, Issue 3, 2009, Pages 1059-1071

  Del Burgo, C ^a   Martin E L ^b,c   Zapatero Osorio, M R ^b   Hauschildt, P H ^d  

^a DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c UNIVERSITY OF CENTRAL FLORIDA   (United States)

^d UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Stars: atmosphers; Stars: fundamental parameters; Stars: low mass, brown dwarfs

Indexed keywords

DUST GRAINS; ECHELLE; EFFECTIVE TEMPERATURE; EVOLUTIONARY MODELS; HIGH RESOLUTION; METALLICITIES; NEAR INFRARED; NEAR INFRARED SPECTRA; NIRSPEC; PHYSICAL PARAMETERS; ROOT MEAN SQUARE; ROTATIONAL VELOCITY; SPECTRAL TYPES; STARS: FUNDAMENTAL PARAMETERS; STARS: LOW-MASS, BROWN DWARFS; SURFACE GRAVITY; SYNTHETIC MODELS;

ANOXIC SEDIMENTS; ASTROPHYSICS; DUST; ESTIMATION; INFRARED DEVICES; SPECTROSCOPY; STARS; TEMPERATURE; UNCERTAINTY ANALYSIS;

GRAVITATION;

EID: 70349677067     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200810752     Document Type: Article

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