Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apjs...99..107c&link_type=abstract
Astrophysical Journal Supplement v.99, p.107
Astronomy and Astrophysics
Astronomy
73
Ism: Clouds, Ism: Kinematics And Dynamics, Ism: Molecules
Scientific paper
We report the results of a survey at very high spectral resolution of interstellar CH and CH+ in diffuse clouds toward 20 bright stars, and medium-resolution observations to determine radial velocities. The high-resolution observations [(λ/δλ) ˜ 500,000] resolve all the CH+ and all the CH lines. Most of the CH lines show multiple overlapping components at this resolution. It is often possible to associate a weak broad CH component with a CH+ component of similar radial velocity and width. The implications of these results for CH and CH+ formation scenarios are discussed.
Crane Philippe
Lambert David L.
Sheffer Yaron
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