On the hypothesis of H2 as the carrier of the diffuse interstellar bands
โ Scribed by P.C. Hinne; W. Ubachs
- Publisher
- Elsevier Science
- Year
- 1995
- Tongue
- English
- Weight
- 381 KB
- Volume
- 240
- Category
- Article
- ISSN
- 0009-2614
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โฆ Synopsis
In a laboratory experiment, employing an extreme ultraviolet/near-infrared double resonance technique, a recent hypothesis by Sorokin and Glownia on the carrier of the diffuse interstellar bands is tested. Quantum states C 1 รท H u, v = 9, J = 1-3 of molecular hydrogen were populated by an extreme ultraviolet laser at 86 nm and used as absorber states for a second excitation step. In transitions to autoionizing doubly excited states of H 2 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.
๐ SIMILAR VOLUMES
It has been proposed that some of the diffuse interstellar absorption bands which have puzzled astronomers for several decades may be assigned to transitions in vibrationally excited H 2 molecules. These molecules would arise in circumstellar environments where stellar Lyman-cx photons create a popu
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