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High-resolution Infrared Spectrum Of The Diatomic Vanadium Oxide
Döring, Eileen
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https://hdl.handle.net/2142/116971
Description
- Title
- High-resolution Infrared Spectrum Of The Diatomic Vanadium Oxide
- Author(s)
- Döring, Eileen
- Contributor(s)
- Fuchs, Guido W.
- Giesen, Thomas
- Breier, Alexander A.
- Blum, Luisa
- Issue Date
- 2022-06-24
- Keyword(s)
- Astronomy
- Abstract
- Small molecules made of refractory materials are thought to play an important role in the dust formation processes around late-type stars. Likewise, they take part in the opacity process of variable late-type stars, as has been shown for the molecule TiO.\footnote{M.J. Reid \& J.E. Goldston, The Astrophysical Journal \textbf{568}, 931 (2002)} Because of similar formation conditions, the diatomic molecule vanadium oxide (VO) is thought to occur in similar locations around stars as TiO.\footnote{L.K. McKemmish \textit{et al.}, Monthly Notices of the Royal Astronomical Society \textbf{463}, 771 (2016)} VO has already been detected in the near-infrared region in the envelope of the red hypergiant VY CMa\footnote{J. Bernal \textit{et al.}, 74th International Symposium on Molecular Spectroscopy (2019)}, but due to the lack of high-resolution laboratory spectra, no astrophysical search of VO in the mid-IR region has been performed. In this work, we report the ro-vibrational absorption spectrum of \(X^4\Sigma^-\) VO, including its hyperfine structure. In our experiment we used a frequency modulated quantum cascade laser in combination with Herriott-type multipass optics. The molecules were produced by laser ablation of a vanadium rod and an N\(_2\)O/He buffer gas, which was subsequently adiabatically expanded into a vacuum chamber. The rotationally cooled spectrum was analyzed using the pgopher software and the molecular constants were determined. The experimental data as well as line predictions will enable a dedicated search for this molecule in space at mid-IR wavelengths.
- Publisher
- International Symposium on Molecular Spectroscopy
- Type of Resource
- text
- Language
- eng
- Handle URL
- https://hdl.handle.net/2142/116971&&
- DOI
- https://doi.org/10.15278/isms.2022.FG11
- Copyright and License Information
- Copyright 2022 held by the authors
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