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Infrared spectroscopy interstellar molecule detection

We have already discussed the high-resolution spectroscopy of the OH radical at some length. It occupies a special place in the history of the subject, being the first short-lived free radical to be detected and studied in the laboratory by microwave spectroscopy. The details of the experiment by Dousmanis, Sanders and Townes [4] were described in section 10.1. It was also the first interstellar molecule to be detected by radio-astronomy. In chapter 8 we described the molecular beam electric resonance studies of yl-doubling transitions in the lowest rotational levels, and in chapter 9 we gave a comprehensive discussion of the microwave and far-infrared magnetic resonance spectra of OH. Our quantitative analysis of the magnetic resonance spectra made use of the results of pure field-free microwave studies of the rotational transitions, which we now describe. [Pg.788]

Table 2.3 List of detected interstellar and circumstellar molecules, radicals and ions, grouped by the number of atoms (N) they contain. Species detected with UV, visible or infrared spectroscopy are indicated in italics... Table 2.3 List of detected interstellar and circumstellar molecules, radicals and ions, grouped by the number of atoms (N) they contain. Species detected with UV, visible or infrared spectroscopy are indicated in italics...

See other pages where Infrared spectroscopy interstellar molecule detection is mentioned: [Pg.325]    [Pg.31]    [Pg.246]    [Pg.159]    [Pg.23]    [Pg.204]   


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