A survey of interstellar C I - Insights on carbon abundances, UV grain albedos, and pressures in the interstellar medium

Details A survey of interstellar C I - Insights on carbon abundances, UV grain albedos, and pressures in the interstellar medium A survey of interstellar C I - Insights on carbon abundances, UV grain albedos, and pressures in the interstellar medium

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231...55j&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, July 1, 1979, p. 55-72.

Astronomy and Astrophysics

Astrophysics

175

Carbon, Interstellar Matter, Satellite Observation, Abundance, Albedo, Hydrogen Clouds, Ultraviolet Spectroscopy

Scientific paper

Interstellar atomic carbon has been sampled over 33 different paths with visual extinctions ranging from about 0.15 to 1.5 mag. The trend of C I vs different forms of hydrogen is found to be steep and somewhat erratic. It is concluded that the observed behavior can be explained by strong differences in the responses of C I, H I, and H2 equilibria to physical conditions, together with marked variations of these conditions within different interstellar clouds.

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