Accretion in ρ ophiuchus brown dwarfs: Infrared hydrogen line ratios

Astronomy and Astrophysics

Volumn 460, Issue 2, 2006, Pages 547-553

  Gatti, T ^a,b   Testi, L ^a   Natta, A ^a   Randich, S ^a   Muzerolle, J ^c  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b UNIVERSITY OF FLORENCE   (Italy)

^c UNIVERSITY OF ARIZONA   (United States)

Author keywords

Accretion, accretion disks; Stars: formation; Stars: low mass, brown dwarfs

Indexed keywords

HYDROGEN; INFRARED RADIATION; MAGNETIC FIELDS; MAGNETOSPHERE; MATHEMATICAL MODELS; THERMAL EFFECTS;

ACCRETION DISKS; ACCRETION RATE; BROWN DWARFS; HYDROGEN LINE RATIOS;

ASTROPHYSICS;

EID: 33845457211     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066095     Document Type: Article

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