UV-controlled physical and chemical structure of protoplanetary disks View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2011-03-09

AUTHORS

V. V. Akimkin, Y. N. Pavlyuchenkov, A. I. Vasyunin, D. S. Wiebe, M. S. Kirsanova, T. Henning

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.

PAGES

33-38

References to SciGraph publications

  • 2008-11. Molecular structure of brown-dwarf disks in ASTRONOMY REPORTS
  • 2003-09. Peculiarities of the UV continuum energy distribution for T Tauri stars in ASTRONOMY LETTERS
  • 2008-05-30. WSO-UV—ultraviolet mission for the next decade in ASTROPHYSICS AND SPACE SCIENCE
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s10509-011-0652-7

    DOI

    http://dx.doi.org/10.1007/s10509-011-0652-7

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1037921450


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