Simulating HII Emission with a Sphere and Shell Model

Details Simulating HII Emission with a Sphere and Shell Model Simulating HII Emission with a Sphere and Shell Model

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20513905k&link_type=abstract

American Astronomical Society Meeting 205, #139.05; Bulletin of the American Astronomical Society, Vol. 36, p.1574

Astronomy and Astrophysics

Astronomy

Scientific paper

The continuum and recombination line emission of HII regions were modeled with a series of increasingly more physically acurate geometrical models: a box, a sphere, and a sphere with a shell. The ionized hydrogen sphere surrounded by a partially ionized shell of different temperature and density in pressure equilibrium can match the recombination line emission of actual HII regions. This model only works when considered under non-LTE conditions.

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