The gas dynamics of H II regions. I - The champagne model

Details The gas dynamics of H II regions. I - The champagne model The gas dynamics of H II regions. I - The champagne model

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....71...59t&link_type=abstract

Astronomy and Astrophysics, vol. 71, no. 1-2, Jan. 1979, p. 59-65.

Astronomy and Astrophysics

Astrophysics

313

Astronomical Models, Gas Dynamics, H Alpha Line, H Ii Regions, Stellar Evolution, Gas Ionization, Hydrogen Ions, Line Shape, Velocity Distribution

Scientific paper

Numerical models of the evolution of H II regions are presented, taking into account the fact that star formation occurs inside a dense cloud. The gas dynamical effects produced after the ionization of the cloud's edge, (from the inside) are here postulated to determine the size, velocity field, and large scale density variation observed in some H II regions. The consequences and observational predictions of these models are also given.

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