Interpretation of the 4141 inverse centimeters (2.415 microns) interstellar infrared absorption feature

Details Interpretation of the 4141 inverse centimeters (2.415 microns) interstellar infrared absorption feature Interpretation of the 4141 inverse centimeters (2.415 microns) interstellar infrared absorption feature

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...431l.135b&link_type=abstract

The Astrophysical Journal, vol. 431, no. 2, pt. 2, p. L135-L138

Astronomy and Astrophysics

Astrophysics

19

Adsorption, Infrared Spectra, Interplanetary Dust, Molecular Interactions, Absorption Spectra, Astronomical Spectroscopy, Energy Of Formation, Monte Carlo Method

Scientific paper

The recently discovered 4141 cm-1 interstellar infrared
feature is argued to be a Q1(0) absorption of para-hydrogen.
Adsorption of H2 by microporous amorphous ice mantles is discussed as a
possible source of the feature.

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