The electron density in the direction of zeta OPH

Details The electron density in the direction of zeta OPH The electron density in the direction of zeta OPH

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..32..211s&link_type=abstract

Astrophysics and Space Science, vol. 32, Jan. 1975, p. 211-213.

Astronomy and Astrophysics

Astrophysics

2

Electron Density Profiles, Hydrogen Clouds, Interstellar Gas, Photoionization, Photodissociation, Ultraviolet Radiation, Vibrational Spectra

Scientific paper

It is shown that photoionization of vibrationally excited H2 and photodissociation of the H2(+) ions produced thereby constitute a significant electron production route in high UV flux situations. A significant fraction of the electron density in the direction of zeta Oph (-15 km per sec cloud) deduced from observations may be expected to arise in this way.

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