The A1II - X1(Epsilon) electronic band of the CH(+) ion has been used as a probe of the physical and dynamical conditions of the ISM for 65 years. In spite of being one of the first molecular species observed in the ISM and the very large number of subsequent observations with large derived column densities, the pure rotational spectra of CH+ has remained elusive in both the laboratory and in the ISM as well. We report the first laboratory measurement of the pure rotation of the CH(+) ion and discuss the detection of CH-13(+) in the ISM. Also reported are the somewhat unexpected chemical conditions that resulted in laboratory production
International audienceWe report the probable detection of the 13CH+ (1-0) line in absorption against...
The z = 0.89 molecular absorber toward PKS 1830-211 provides us with the opportunity to probe the ch...
The formation of CH+ in the interstellar medium (ISM) has long been an outstanding problem in chemic...
Author Institution: Jet Propulsion Laboratory, California Institute; of Technology, Pasadena, CA 911...
5 pags., 2 figs., 5 tabs.C-H stretches of the fundamental ions CH and CH, which have long been searc...
Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Met...
Author Institution: Department of Chemistry and Department of Physics and Astronomy, University of W...
Context. Spectral lines of minor isotopic species of molecules that are abundant in space may also b...
Aims. The HIFI instrument onboard Herschel has allowed high spectral resolution and sensitive observ...
Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Met...
We report the first detection of the ground-state rotational transition of the methylidyne cation CH...
International audienceAims: To follow the species chemistry arising in diverse sources of the Galaxy...
International audienceWe report the probable detection of the 13CH+ (1-0) line in absorption against...
The z = 0.89 molecular absorber toward PKS 1830-211 provides us with the opportunity to probe the ch...
The formation of CH+ in the interstellar medium (ISM) has long been an outstanding problem in chemic...
Author Institution: Jet Propulsion Laboratory, California Institute; of Technology, Pasadena, CA 911...
5 pags., 2 figs., 5 tabs.C-H stretches of the fundamental ions CH and CH, which have long been searc...
Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Met...
Author Institution: Department of Chemistry and Department of Physics and Astronomy, University of W...
Context. Spectral lines of minor isotopic species of molecules that are abundant in space may also b...
Aims. The HIFI instrument onboard Herschel has allowed high spectral resolution and sensitive observ...
Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Met...
We report the first detection of the ground-state rotational transition of the methylidyne cation CH...
International audienceAims: To follow the species chemistry arising in diverse sources of the Galaxy...
International audienceWe report the probable detection of the 13CH+ (1-0) line in absorption against...
The z = 0.89 molecular absorber toward PKS 1830-211 provides us with the opportunity to probe the ch...
The formation of CH+ in the interstellar medium (ISM) has long been an outstanding problem in chemic...