UV fluorescence of molecular hydrogen and red dust emission in the Gamma Cassiopeiae nebula IC 63

Details UV fluorescence of molecular hydrogen and red dust emission in the Gamma Cassiopeiae nebula IC 63 UV fluorescence of molecular hydrogen and red dust emission in the Gamma Cassiopeiae nebula IC 63

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336l..21w&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. L21-L24.

Astronomy and Astrophysics

Astronomy

44

Fluorescence, Hydrogen Clouds, Interstellar Matter, Reflection Nebulae, Ultraviolet Astronomy, Cosmic Dust, Iue, Ultraviolet Spectra

Scientific paper

Resonant fluorescence of molecular hydrogen has been observed in the
reflection nebula IC 63 with the IUE satellite. Both the noncoherent
resonant scattering and the dissociative continuum are shown to agree
well with molecular theory. Extended red emission is also found in this
nebula and may be physically related to the dissociation of H2.

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