The Detectability of Molecular Hydrogen in Interstellar Space

Details The Detectability of Molecular Hydrogen in Interstellar Space The Detectability of Molecular Hydrogen in Interstellar Space

May 1966

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1966ssrv....5..419v&link_type=abstract

Space Science Reviews, Volume 5, Issue 3, pp.419-434

Physics

4

Scientific paper

This review consists essentially of three parts where we consider: (1) the structure and spectrum of the hydrogen molecule; (2) the processes that in interstellar space can lead to the forma-tion and to the dissociation of the hydrogen molecule, with the aim of establishing its abundance, both on the average and in particular regions of the Galaxy; (3) the lines originating from interstellar molecular hydrogen that could be observed from the Earth. In this last Section the possible obser-vations are classified from the point of view of the height in the atmosphere from which they have to be made.

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