Astrophysics and Space Science

, Volume 216, Issue 1–2, pp 143–150 | Cite as

Highly supersonic molecular flows in wind-clump boundary layers

  • M. T. Malone
  • J. E. Dyson
  • T. W. Hartquist
Article

Abstract

The gradual acceleration, through viscous coupling to a wind, of molecular hydrogen in turbulent boundary layers around obstacle clumps is proposed to be responsible for the widths of the emission features with full widths at zero intensity of greater than 100 km s−1.

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Copyright information

© Kluwer Academic Publishers 1994

Authors and Affiliations

  • M. T. Malone
    • 1
  • J. E. Dyson
    • 1
  • T. W. Hartquist
    • 2
  1. 1.Department of Physics and AstronomyThe University of ManchesterManchesterEngland
  2. 2.Max Planck Institute for Extraterrestrial PhysicsGarchingGermany

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