Turbulence in the Ursa Major cirrus cloud

Details Turbulence in the Ursa Major cirrus cloud Turbulence in the Ursa Major cirrus cloud

1998-04-21

arxiv.org/abs/astro-ph/9804209v1

Astronomy and Astrophysics

Astrophysics

5 pages, 4 figures, to be published in 'Interstellar Turbulence', Puebla, 1998, Cambridge University Press, Pepe Franco and Al

Scientific paper

High resolution 21 cm observations of the Ursa Major cirrus revealed highly filamentary structures down to the 0.03 pc resolution. These filaments, still present in the line centroid map, show multi-Gaussian components and seem to be associated with high vorticity regions. Probability density functions of line centroid increments and structure functions were computed on the line centroid field, providing strong evidences for the presence of turbulence in the atomic gas.

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