Molecular hydrogen emission from star-forming regions in the Large Magellanic Cloud.

Details Molecular hydrogen emission from star-forming regions in the Large Magellanic Cloud. Molecular hydrogen emission from star-forming regions in the Large Magellanic Cloud.

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989msngr..56...57b&link_type=abstract

The Messenger, vol. 56, p. 57-59

Physics

Magellanic Clouds: Star-Forming Regions, Magellanic Clouds: Molecular Hydrogen

Scientific paper

Molecular hydrogen is probably the most abundant molecule of the
interstellar medium. Giant molecular clouds consist mainly of H2.
There are limited possibilities for direct observations of the H,
molecule.

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