Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....54..517t&link_type=abstract
Astronomy and Astrophysics, vol. 54, no. 2, Jan. 1977, p. 517-524.
Astronomy and Astrophysics
Astrophysics
16
Astrophysics, Globules, H Ii Regions, Ionization, Shock Wave Propagation, Gas Density, Isotropic Media, Reflected Waves, Time Response
Scientific paper
The motion of ionization fronts into globules in H II regions is studied numerically to show how the globules evolve, why they persist, and whether the overall flow pattern approaches the flow conditions described analytically by previous authors. The time evolution of the interaction between various weak R-type fronts and globules immersed in constant-density clouds is analyzed in three different cases. The results suggest that globules with a core of neutral gas can exist for long periods in H II regions, such a core should be surrounded by a region of ionized gas that may be observable as a bright-rim structure, and the normally assumed hydrostatic-equilibrium condition is violated by the appearance of shocks in the flow. It is also found that the ionized gas ultimately streams away from the condensations; that the ionizing flux is heavily attenuated in the ionized region, producing a very slow weak D-front; and that the surrounding ionization front should evolve very rapidly in the case of high-density condensations, leading to the immediate appearance of shocks in the flow and to a stationary weak D-front.
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