A comparison of chemistry and dust cloud formation in ultracool dwarf model atmospheres

Monthly Notices of the Royal Astronomical Society

Volumn 391, Issue 4, 2008, Pages 1854-1873

  Helling, Ch ^a   Ackerman, A ^b   Allard, F ^c,d   Dehn, M ^e   Hauschildt, P ^e   Homeier, D ^f   Lodders, K ^g   Marley, M ^h   Rietmeijer, F ⁱ   Tsuji, T ^j   Woitke, P ^k  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b NASA GODDARD INSTITUTE FOR SPACE STUDIES   (United States)

^c UNIVERSITÉ DE LYON   (France)

^d CNRS   (France)

^e UNIVERSITY OF HAMBURG   (Germany)

^f UNIVERSITY OF GÖTTINGEN   (Germany)

^g WASHINGTON UNIVERSITY   (United States)

^h NASA AMES RESEARCH CENTER   (United States)

ⁱ UNIVERSITY OF NEW MEXICO   (United States)

^j UNIVERSITY OF TOKYO   (Japan)

^k UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

more..

Author keywords

Stars: atmospheres; Stars: low mass, brown dwarfs

Indexed keywords

ASTROPHYSICS; ATMOSPHERIC CHEMISTRY; ATMOSPHERIC TEMPERATURE; DUST; INFRARED DEVICES; IRON COMPOUNDS; OPACITY; STARS; TESTING; UNCERTAINTY ANALYSIS;

CLOUD FORMATION; CLOUD MODELING; DUST CLOUDS; MODEL ATMOSPHERE; MODELING APPROACH; OXIDE IRON; STARS: ATMOSPHERE; STARS: LOW-MASS BROWN DWARFS; SUBSTELLAR OBJECTS; TEST CASE;

SILICATES;

EID: 57649130969     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13991.x     Document Type: Article

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