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pro vyhledávání: '"Carballido, Augusto"'
(Abridged) We perform the first study of magnetohydrodynamic processes in the protolunar disk (PLD). With the use of published data on the chemical composition of the PLD, along with existing analytical models of the disk structure, we show that the
Externí odkaz:
http://arxiv.org/abs/1512.06194
We analyze the coagulation of dust in and around a gap opened by a Jupiter-mass planet. To this end, we carry out a high-resolution magnetohydrodynamic (MHD) simulation of the gap environment, which is turbulent due to the magnetorotational instabili
Externí odkaz:
http://arxiv.org/abs/1512.03945
Autor:
Carballido, Augusto
(Abridged) Numerical magnetohydrodynamic (MHD) simulations of a turbulent solar nebula are used to study the growth of dust mantles swept up by chondrules. A small neighborhood of the solar nebula is represented by an orbiting patch of gas at a radiu
Externí odkaz:
http://arxiv.org/abs/1012.0324
Autor:
Carballido, Augusto, Lee, William H.
The central engine of Gamma Ray Bursts is hidden from direct probing with photons mainly due to the high densities involved. Inferences on their properties are thus made from their cosmological setting, energetics, low-energy counterparts and variabi
Externí odkaz:
http://arxiv.org/abs/1011.5515
We perform numerical simulations of solid particle motion in a shearing box model of a protoplanetary disc. The accretion flow is turbulent due to the action of the magnetorotational instability. Aerodynamic drag on the particles is modelled using th
Externí odkaz:
http://arxiv.org/abs/0801.3646
Publikováno v:
Mon.Not.Roy.Astron.Soc.358:1055,2005
We calculate the radial diffusion coefficient for a passive contaminant in an accretion disc which is turbulent due to the action of the magnetorotational instability. Numerical MHD simulations are used to follow the evolution of a local patch of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0501474
Publikováno v:
In Icarus April 2016 268:89-101
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Akademický článek
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