Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008a%26a...479..149w&link_type=abstract
Astronomy and Astrophysics, Volume 479, Issue 1, February III 2008, pp.149-154
Astronomy and Astrophysics
Astrophysics
12
Ism: Molecules, Ism: Abundances
Scientific paper
Observations of interstellar absorption bands of CH+ molecule at 3957 and 4232 Å were applied to determine column densities toward 53 stars. The targets were selected because the atomic and molecular hydrogen column densities are published. The data on CH+ were acquired using four echelle spectrographs situated in both the Northern and Southern hemispheres. Spatial relations between column densities of CH+ and those of molecular, atomic and total hydrogen show large scatter, suggesting there is no relation between abundances of methylidyne cation and hydrogen in any form.
Galazutdinov Gazinur
Krełowski Jacek
Musaev Faig
Weselak T.
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