Detectability of dirty dust grains in brown dwarf atmospheres

Astronomy and Astrophysics

Volumn 451, Issue 2, 2006, Pages

  Helling, Ch ^a   Thi, W F ^a,c   Woitke, P ^b   Fridlund, M ^a  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b LEIDEN UNIVERSITY   (Netherlands)

^c UNIVERSITY OF EDINBURGH   (United Kingdom)

Author keywords

Astrochemistry; Infrared: stars; Methods: numerical; Stars: atmospheres; Stars: low mass, brown dwarfs

Indexed keywords

AMORPHOUS SILICON; ASTROPHYSICS; GRAIN GROWTH; GRAIN SIZE AND SHAPE; HEAT TRANSFER;

ASTROCHEMISTRY; DUST FORMATION THEORY; INFRARED: STARS; METHODS: NUMERICAL; STARS: ATMOSPHERES; STARS: LOW-MASS, BROWN DWARFS;

SPACE RESEARCH;

EID: 33646806472     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064944     Document Type: Article

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