Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21344101t&link_type=abstract
American Astronomical Society, AAS Meeting #213, #441.01; Bulletin of the American Astronomical Society, Vol. 41, p.317
Astronomy and Astrophysics
Astronomy
1
Scientific paper
A basic process concentrating the heavy elements during planet formation is the settling of primordial dust particles in protostellar disks due to the component of the stellar gravity perpendicular to the disk plane. The effectiveness of the settling depends on the strength and distribution of turbulence in the disk gas. The magneto-rotational instability drives turbulence only in active layers near the top and bottom surfaces of the disk where stellar X-rays produce sufficient ionization for good coupling of the gas to magnetic fields. Much of the disk interior remains laminar and is a so-called dead zone. We explore the consequences of the dead zone for grain settling and disk evolution. Recombination on the grain surfaces is efficient, so that the movements of the particles relative to the gas determine whether the active layers (1) grow over time through reduced recombination rates as grains are lost by settling, (2) shrink over time as the turbulence lifts grains out of the dead zone, or (3) vary episodically. We make 3-D stratified shearing-box resistive MHD calculations, tracking the movements of the grains and solving a time-dependent ionization-recombination reaction network, so that the back-reaction of the dust on the electrical resistivity of the gas is explicitly included. We examine how the dead zone governs the distribution of the grains through the disk thickness, and how the grains in turn affect the dead zone size and the flow of gas through the disk to the star.
Carballido Augusto
Sano Takayoshi
Turner Neal James
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