On the evolution of ionized gas around hot stars

Details On the evolution of ionized gas around hot stars On the evolution of ionized gas around hot stars

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..41...39m&link_type=abstract

Astrophysics and Space Science, vol. 41, May 1976, p. 39-56.

Astronomy and Astrophysics

Astrophysics

6

Gas Evolution, Hot Stars, Ionized Gases, Stellar Atmospheres, Finite Difference Theory, Forbidden Transitions, Gas Ionization, H Ii Regions, Line Spectra, Optical Thickness, Stellar Evolution, Stellar Models

Scientific paper

The initial evolution of a uniform H II region around a star of 36 solar
masses is described. The general equations of the problem are solved
numerically by a finite-difference method. Forbidden-line emission by
ions of C, N, O, and Ne is taken into account.

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