The role of convection, overshoot, and gravity waves for the transport of dust in M dwarf and brown dwarf atmospheres

Astronomy and Astrophysics

Volumn 513, Issue 4, 2010, Pages

  Freytag, B ^a   Allard, F ^a,b   Ludwig, H G ^c   Homeier, D ^d   Steffen, M ^e  

^a UNIVERSITÉ DE LYON   (France)

^b INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d UNIVERSITY OF GÖTTINGEN   (Germany)

^e ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Brown dwarfs; Convection; Hydrodynamics; Stars: atmospheres; Stars: low mass; Waves

Indexed keywords

ATMOSPHERICS; CLOUDS; DUST; FLUID DYNAMICS; GRAVITATIONAL EFFECTS; GRAVITY WAVES; HYDRODYNAMICS; MIXING; TEMPERATURE; TWO DIMENSIONAL; WAVES;

BROWN DWARFS; CHEMICAL COMPOSITIONS; CLOUD FORMATION; CONVECTION ZONE; CONVECTIVE FLOW; DUST CLOUDS; DUST GRAINS; DUST LAYER; EFFECTIVE TEMPERATURE; MACROSCOPIC FLOW; MIXING MATERIALS; MIXING PROCESS; MIXING PROPERTY; RADIATION HYDRODYNAMICS SIMULATION; SMALL SCALE; SPATIAL SCALE; STANDARD MODEL; STARS: ATMOSPHERE; STARS: ATMOSPHERES; STARS: LOW MASS; STELLAR SURFACES;

STARS;

EID: 77951120776     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913354     Document Type: Article

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