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Prospective work for Alma, Herschel, Sofia : submillimeter-wave spectroscopy of complex organic molecules

Published online by Cambridge University Press:  13 February 2013

T.R. Huet ,
L. Margulès ,
R.A. Motiyenko ,
S. Bailleux ,
M. Goubet  and
G. Wlodarczak
T.R. Huet
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]
L. Margulès
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]
R.A. Motiyenko
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]
S. Bailleux
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]
M. Goubet
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]
G. Wlodarczak
Affiliation:
Laboratoire PhLAM, Bât. P5, CNRS UMR 8523, Université Lille 1, 59655 Villeneuve d’Ascq Cedex, France;. e-mail: [email protected]

Abstract

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Laboratory analysis of spectra of potential interstellar molecules from the radio-frequency to the THz range is a prerequisite for their subsequent identification by radioastronomical techniques. The spectral analysis allows us to derive molecular parameters that are able to model the frequency and intensity patterns of the transitions, as well as to predict with a high degree of precision the frequencies of transitions not measured in the laboratory.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 58: ECLA - European Conference on Laboratory Astrophysics , 2012 , pp. 263 - 266
Copyright
© The Author(s) 2013

References

Références

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