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The microwave spectroscopy of HCOO13CH3 in the second torsional excited state
Kobayashi, Kaori
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https://hdl.handle.net/2142/97018
Description
- Title
- The microwave spectroscopy of HCOO13CH3 in the second torsional excited state
- Author(s)
- Kobayashi, Kaori
- Contributor(s)
- Fujitake, Masaharu
- Ohashi, Nobukimi
- Urata, Yuki
- Kuwahara, Takuro
- Issue Date
- 2017-06-21
- Keyword(s)
- Astronomy
- Date of Ingest
- 2017-07-27T20:15:32Z
- 2018-01-29T23:05:57Z
- Abstract
- Methyl formate (HCOOCH$_3$) is an abundant interstellar molecule, found almost everywhere in the star-forming region. _x000d_ The interstellar abundance of the $^{13}$C is about 1/50 of $^{12}$C. _x000d_ The $^{13}$C substituted methyl formate in the ground and first excited states were already found toward massive star-forming_x000d_ regions including Orion KL. _x000d_ $footnote{C. Favre, M. Carvajal, D. Field, J. K. J$o$rgensen, S. E. Bisschop, N. Brouillet, D. Despois, A. Baudry, I. Kleiner, E. A. Bergin, N. R. Crockett, J. L. Neill, L. Margu`{e}s, T. R. Huet, and J. Demaison,_x000d_ textit{Astrophys. J. Suppl. Ser.} underline{textbf{215}}, 25 (2014).}$_x000d_ With the aid of the state-of-the-art telescope like ALMA,_x000d_ the pure rotational transitions in the second torsional excited may be identified in the near future and laboratory data are necessary. _x000d_ We recorded the spectra of HCOOCH$_3$ below 340 GHz by using conventional source-modulation microwave spectrometer._x000d_ The assignment of the pure rotational spectra in the second torsional excited state_x000d_ and the analysis by using pseudo-PAM Hamiltonian, which was effective to analyze the normal species, will be reported. _x000d_
- Publisher
- International Symposium on Molecular Spectroscopy
- Type of Resource
- text
- Genre of Resource
- Conference Paper / Presentation
- Language
- eng
- Permalink
- http://hdl.handle.net/2142/97018
- DOI
- https://doi.org/10.15278/isms.2017.WA02
- Copyright and License Information
- Copyright 2017 Kaori Kobayashi
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