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The methylidyne ion CH+ was one of the first molecules detected in the interstellar medium, being identified in absorption at visible/near ultraviolet wavelengths in the spectra of background stars in 1941 by Douglas and Herzberg. CH+ emission at visible wavelengths is seen from the tails of comets. Pure rotational transitions have been observed at far infrared wavelengths from planetary nebula, molecular clouds, and Photodissociation regions using the ISO and Herschel satellites.
References and Further Reading
Cernicharo J, Liu XW, Gonzalez-Alfonso E, Cox P, Barlow MJ, Lim T, Swinyard BM (1997) Discovery of far-infrared pure rotational transitions of CH+ in NGC 7027. Astrophys J Lett 483:L65–L68
Douglas AE, Herzberg G (1941) Note on CH+ in interstellar space and in the laboratory. Astrophys J 94:381
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© 2014 Springer-Verlag Berlin Heidelberg
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Irvine, W.M. (2014). Methylidyne Cation. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1809-4
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1809-4
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Publisher Name: Springer, Berlin, Heidelberg
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