Two-dimensional radiation-hydrodynamics calculations of the formation of the O-B associations in dense molecular clouds

Details Two-dimensional radiation-hydrodynamics calculations of the formation of the O-B associations in dense molecular clouds Two-dimensional radiation-hydrodynamics calculations of the formation of the O-B associations in dense molecular clouds

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..275k&link_type=abstract

(International Astronomical Union, Colloquium on Stellar Hydrodynamics, 58th, Los Alamos, N. Mex., Aug. 12-15, 1980.) Space Scie

Astronomy and Astrophysics

Astronomy

17

B Stars, Hydrodynamic Equations, Interstellar Gas, Molecular Clouds, O Stars, Radiative Transfer, Stellar Evolution, Early Stars, Gas Density, Ionizing Radiation, Shock Fronts

Scientific paper

Two-dimensional calculations of ionization-shockwave propagation into a
curved molecular cloud are presented. Density enhancement occurs due to
the combined effects of cloud curvature and radiation flow. The star
formation process is expected to be enhanced near the edges of
irregularly shaped molecular clouds.

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