Dynamics of bipolar ionization cones

Details Dynamics of bipolar ionization cones Dynamics of bipolar ionization cones

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...245..257b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 245, no. 1, May 1991, p. 257-261.

Astronomy and Astrophysics

Astrophysics

3

Gas Ionization, H Ii Regions, Nebulae, Radiation Distribution, Active Galactic Nuclei, Recombination Reactions, Star Formation, Ultraviolet Spectra

Scientific paper

This paper considers the evolution of the ionized region produced by a source of UV photons where the emitted radiation is confined to a cone, rather than emerging isotropically. The ionization fronts at the end of such conical HII regions travel faster, and propagate to greater distances, than in the spherical case. The model is applied to recent observations of NGC 6334(A).

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