Radiation-hydrodynamics of HII regions and molecular clouds

Details Radiation-hydrodynamics of HII regions and molecular clouds Radiation-hydrodynamics of HII regions and molecular clouds

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8214032s&link_type=abstract

Presented at the IAU Colloq., Penticton, Canada, 24-26 Jun. 1981

Physics

H Ii Regions, Implosions, Molecular Clouds, Stellar Evolution, Cosmology, Herbig-Haro Objects, Ionization, Masers, Shock Fronts

Scientific paper

Two-dimensional calculations of ionization-shock fronts surrounding neutral cloud clumps reveal that a radiation-driven implosion of the clump can occur. The implosion of a cloud clump results in the formation of density enhancements that may eventually form low mass stars. The smaller globules produced may become Herbig-Haro objects, or maser sources.

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