Photoionization rates in the interstellar medium

Details Photoionization rates in the interstellar medium Photoionization rates in the interstellar medium

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.206..449k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 206, Jan. 15, 1984, p. 449-452.

Astronomy and Astrophysics

Astronomy

13

Gas Ionization, Hydrogen Clouds, Interstellar Gas, Ion Production Rates, Photoionization, Interstellar Radiation, Molecular Clouds

Scientific paper

The Gondhalekar et al. (1980) determination of the radiation field from 2740 A down to the Lyman limit at 912 A is the basis of the present calculation of photoionization rates for several species that are of importance in the interstellar medium. The results obtained are compared with previous estimates by De Boer et al. (1973). It is noted that large radiation field variations will occur in regions of space near OB associations or within dense dust clouds, with corresponding effects on the photoionization rates.

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