The CO Cameron band emission in the Red Rectangle

Details The CO Cameron band emission in the Red Rectangle The CO Cameron band emission in the Red Rectangle

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mnras.313l..17y&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 313, Issue 2, pp. L17-L18.

Astronomy and Astrophysics

Astronomy

3

Molecular Processes, Ism: Individual: Red Rectangle, Ultraviolet: Ism

Scientific paper

The origin of the strong CO Cameron band emission in the Red Rectangle is investigated. From a comparison of laboratory spectroscopic data and astronomical observations in combination with chemical modelling, it is concluded that the Cameron band emission of CO originates from the dissociative recombination of HCO+, and its intensity provides a measure of the product of the density of HCO+ ions and the electron density, integrated along the line of sight.

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