Turbulence in the Ursa Major IR cirrus cloud
M. A. Miville-Deschênes, G. Joncas, F. Boulanger;
In Interstellar Turbulence, 1998, Proceedings of the 2nd Guillermo Haro Conference, held in Puebla, Mexico, Cambridge University Press, Franco, J. and Carraminana, A., p. 24
ABSTRACT:High resolution 21 cm observations revealed highly filamentary structures down to the 0.1pc resolution
in the $T_B$ maps of the Ursa Major cirrus.
These filaments are still
present in the velocity field maps.
A statistical analysis of the velocities
was done and compared to recent numerical simulations.
This work is part
of a more general analysis on the kinematical and turbulent behavior of
the atomic gas and its influence on dust evolution.
PERSOKEY:turbulence, cirrus, h_i, iso, pah, mir, 21 cm, dust, statistical analysis, ,
CODE: miville-deschenes98a