Heating and ionization of the intercloud medium

Details Heating and ionization of the intercloud medium Heating and ionization of the intercloud medium

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..161c&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

B Stars, Gas Ionization, Interstellar Matter, O Stars, Planetary Nebulae, Stellar Radiation, Black Body Radiation, Electron Density (Concentration), Free Electrons, Galactic Radiation, Optical Thickness

Scientific paper

A summary regarding the fundamental data of the intercloud medium is provided, taking into account particles, the radiation from O-B stars, diffuse galactic X rays, optically thin planetary nebulae, and UV stars. It is shown that for the intercloud medium a source of ionization other than O-B stars must exist at high galactic latitudes. Possible reasons for the presence of electrons at high galactic latitudes are considered.

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