On the hypothesis of H2 as the carrier of the diffuse interstellar bands.

Details On the hypothesis of H2 as the carrier of the diffuse interstellar bands. On the hypothesis of H2 as the carrier of the diffuse interstellar bands.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cpl...240..351h&link_type=abstract

Chem. Phys. Lett., Vol. 240, No. 4, p. 351 - 356

Physics

11

Diffuse Interstellar Bands: Laboratory Simulations

Scientific paper

In a laboratory experiment, employing an extreme ultraviolet/near-infrared double resonance technique, a recent hypothesis by Sorokin and Glownia (1995) on the carrier of the diffuse interstellar bands is tested. In transitions to autoionizing doubly excited states of H2 many resonances of strongly varying widths were observed. The frequency positions and linewidths are in general not consistent with the observed diffuse interstellar bands in the range 766 - 788 nm, nor with the predictions of Sorokin and Glownia. However, two lines are found in the present study that do coincide with diffuse interstellar bands.

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