Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...48..299s&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 48, May 1982, p. 299-304.
Astronomy and Astrophysics
Astrophysics
127
Astronomical Catalogs, Astronomical Models, H Ii Regions, Stellar Temperature, Abundance, Computer Programs, Gas Density, Nebulae, O Stars, Photoionization, Tables (Data)
Scientific paper
An extensive grid of model H II regions is presented covering a wide range of stellar effective temperatures and abundances. The gas densities vary from 10 to 1000 per cu cm, including several two-component models. All the models were obtained with a computer code that calculates the ionization and temperature structure of a static nebula photoionized by a hot star, under the assumption of equilibrium for all the microscopic processes.
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