A dataset provided by the European Space Agency

Name OT2_mgerin_6
Title Search for CH2 D+, a key reactant in interstellar chemistry
URL

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DOI https://doi.org/10.5270/esa-lj5jsjt
Author gerin, m.
Description We propose to perform a deep search for the CH2D+ ionwith Herschel/HIFI. This species plays a key role in interstellar chemistry, especially for deuterium fractionation at moderate temperature, but also as tracer of the symmetrical species CH3+.Because of its low dipole moment, and floppy character, its rotational transitions were not accurately known until recently (Amano 2010). Also, only two millimeter transition and onesubmillimeter transition are available from the ground, but inspectral regions where multiple emission lines from other speciesare present. Therefore, this ion escaped detection despite extensive searches bysome of the proponents for over 30 years. Three of the most intense linesof CH2D+ are accessible to Herschel/HIFI in relatively clean spectralregions. The detection of CH2D+ seems therefore to be finally withinreach, providing a key proof of the validity of state of the artchemical networks.
Publication
    Instrument HIFI_HifiPoint_dbs
    Temporal Coverage 2012-09-04T17:12:53Z/2012-09-08T09:31:52Z
    Version SPG v14.1.0
    Mission Description Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
    Creator Contact https://support.cosmos.esa.int/h®erschel/
    Date Published 2013-03-08T09:05:06Z
    Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
    Publisher And Registrant European Space Agency
    Credit Guidelines European Space Agency, gerin et al., 2013, 'Search for CH2 D+ comma a key reactant in interstellar chemistry', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-lj5jsjt