The Amount of CH Produced during CH + Synthesis in Interstellar Clouds

Details The Amount of CH Produced during CH + Synthesis in Interstellar Clouds The Amount of CH Produced during CH + Synthesis in Interstellar Clouds

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apj...481..795f&link_type=abstract

Astrophysical Journal v.481, p.795

Astronomy and Astrophysics

Astronomy

16

Ism: Abundances, Ism: Molecules, Molecular Processes

Scientific paper

A particularly useful constraint for models of CH+ formation in interstellar clouds is knowledge of the amount of CH associated with CH+ synthesis. For lines of sight with no detectable CN absorption, this column of CH can be inferred through a combined analysis of C I excitation and simplified chemical models. The approach is applied to data for two lines of sight, those toward 23 Ori and beta 1 Sco, for which N(CH)/N(CH+) <= 0.40.

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