UV-controlled physical and chemical structure of protoplanetary disks
Earth and Planetary Astrophysics
2015-05-27 v2
Abstract
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.
Keywords
Cite
@article{arxiv.1102.4986,
title = {UV-controlled physical and chemical structure of protoplanetary disks},
author = {V. Akimkin and Ya. Pavlyuchenkov and A. Vasyunin and D. Wiebe and M. Kirsanova and Th. Henning},
journal= {arXiv preprint arXiv:1102.4986},
year = {2015}
}
Comments
Accepted for publication in Astrophysics and Space Science (2011)