Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26as...32..429s&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 32, June 1978, p. 429-438.
Astronomy and Astrophysics
Astrophysics
57
Astronomical Models, Gas Ionization, Gas Temperature, H Ii Regions, Interstellar Gas, Radiative Transfer, Chemical Composition, Diffuse Radiation, Gas Density, Heat Balance, Nebulae, Numerical Integration, Temperature Profiles
Scientific paper
Model H II regions have been constructed by solving the radiative transfer, ionization equilibrium, and thermal balance equations. The varying parameters were the characteristics of the star, the gas density distribution, and its chemical composition. Results are given for the ionization and temperature structure, the emission line spectrum, and the variation of optical depth inside the nebula. The influence of the diffuse radiation is discussed. Particular emphasis is placed on those results which do not fit into the classical picture of an H II region.
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