Origin of extragalactic H2 emission.

Details Origin of extragalactic H2 emission. Origin of extragalactic H2 emission.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996asthe..89..438m&link_type=abstract

Astronomical Herald, Vol. 89, No. 10, p. 438 - 446

Astronomy and Astrophysics

Astronomy

Molecular Hydrogen: Seyfert Galaxies, Molecular Hydrogen: Starburst Galaxies, Molecular Hydrogen: Emission Lines

Scientific paper

The origin of near-infrared H2 emission from Seyfert and
starburst galaxies is still a puzzle. The authors review various
scenarios that have been proposed during the last decade: shock heating,
UV pumping, X-ray heating, UV heating, and formation pumping.

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