Multi-fibre optical spectroscopy of low-mass stars and brown dwarfs in Upper Scorpius

Astronomy and Astrophysics

Volumn 527, Issue 3, 2011, Pages

  Lodieu, N ^a,b   Dobbie, P D ^c   Hambly, N C ^d  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSIDAD DE LA LAGUNA   (Spain)

^c AUSTRALIAN ASTRONOMICAL OBSERVATORY   (Australia)

^d UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

brown dwarfs; open clusters and associations: individual: Upper Scorpius; stars: luminosity function, mass function; techniques: spectroscopic

Indexed keywords

BROWN DWARFS; DEEP-SKY; DIAGNOSTIC FEATURES; EFFECTIVE TEMPERATURE; EQUIVALENT WIDTH; EVOLUTIONARY MODELS; FIELD OF VIEWS; FORMATION MECHANISM; LOW-MASS; LOW-MASS STARS; LUMINOSITY FUNCTIONS; MASS FUNCTIONS; OPEN CLUSTERS; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: UPPER SCORPIUS; OPTICAL SPECTROSCOPY; PROPER MOTION; SIGNAL TO NOISE; SPECTRAL TYPES; SPECTROSCOPIC DATA; STARS: LUMINOSITY FUNCTION, MASS FUNCTION; TECHNIQUES: SPECTROSCOPIC;

INFRARED SPECTROSCOPY; LITHIUM; LUMINANCE; PHOTOMETRY; POTASSIUM IODIDE; SODIUM; SURVEYS;

STARS;

EID: 78751651455     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014992     Document Type: Article

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