Interstellar abundances toward zeta Ophiuchi

Details Interstellar abundances toward zeta Ophiuchi Interstellar abundances toward zeta Ophiuchi

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193l..35m&link_type=abstract

Astrophysical Journal, vol. 193, Oct. 1, 1974, pt. 2, p. L35-L39.

Astronomy and Astrophysics

Astrophysics

231

Absorption Spectra, Abundance, Hydrogen Clouds, Interstellar Gas, Satellite Observation, Stellar Spectra, Astronomical Models, Cosmic Dust, Far Ultraviolet Radiation, Line Spectra, Oao 3, Solar System

Scientific paper

Extensive Copernicus observations of interstellar absorption lines in front of zeta Oph have been combined with similar ground-based data to give column densities or limits on 26 elements in H I clouds. Compared with solar-system abundances, there is a depletion of most elements relative to hydrogen, except S and Zn, by factors of 3 to 4000. The depletions generally are larger for the higher condensation temperatures.

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