Two-Photon Absorption by Hydrogen Molecules: Origin of the 2175 Angstrom Astronomical Band?
The near UV spectra of OB stars in our galaxy are often dominated by a very broad extinction band peaking at ~2175 Angstroms. Forty years after its discovery, the origin of this band remains unknown, although interstellar dust particles are generally assumed to be the carriers. Here we report that t...
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Main Authors | , |
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Format | Journal Article |
Language | English |
Published |
03.08.2006
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Subjects | |
Online Access | Get full text |
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Summary: | The near UV spectra of OB stars in our galaxy are often dominated by a very
broad extinction band peaking at ~2175 Angstroms. Forty years after its
discovery, the origin of this band remains unknown, although interstellar dust
particles are generally assumed to be the carriers. Here we report that
two-photon absorption by hydrogen molecules in gaseous clouds enveloping OB
stars can lead to a band peaking at ~2175 Angstroms. We present astronomical
spectral evidence supporting our proposal that this nonlinear absorption
mechanism accounts for the lambda2175 feature. |
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Bibliography: | LANL LA-UR-06-1898 |
DOI: | 10.48550/arxiv.astro-ph/0608092 |