UV-controlled physical and chemical structure of protoplanetary disks

Details UV-controlled physical and chemical structure of protoplanetary disks UV-controlled physical and chemical structure of protoplanetary disks

2011-02-24

arxiv.org/abs/1102.4986v2

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

Accepted for publication in Astrophysics and Space Science (2011)

Scientific paper

We study details of the UV radiation transfer in a protoplanetary disk,
paying attention to the influence of dust growth and sedimentation on the disk
density and temperature. Also, we show how the dust evolution affects
photoreaction rates of key molecules, like CN and CS.

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