NH_2_CH_2_CN transition frequencies Virtual Observatory Resource

Authors
  1. Degli Esposti C.
  2. Dore L.
  3. Melosso M.
  4. Kobayashi K.
  5. Fujita C.
  6. Ozeki H.
  7. Published by
    CDS
Abstract

It is important to study possible precursors of amino acids such as glycine to enable future searches in interstellar space. Aminoacetonitrile (NH_2_CH_2_CN) is one of the most feasible molecules for this purpose. This molecule was already detected toward Sgr B2(N). Aminoacetonitrile has a few low-lying vibrational excited states, and transitions within these states may be found in space. In this study, the pure-rotational transitions in the three lowest vibrational states in the 80-450 GHz range have been assigned and analyzed. It was found to be very important to include Coriolis coupling between the two lowest vibrational fundamentals, while the third one was unperturbed. The partition function was evaluated considering these new results.

Keywords
  1. atomic-physics
  2. radio-spectroscopy
Bibliographic source Bibcode
2017ApJS..230...26D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/230/26
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJS/230/26
Document Object Identifer DOI
doi:10.26093/cds/vizier.22300026

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/230/26
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/230/26
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/230/26
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2017-08-17T15:40:56Z
Resource record created
2017-08-17T15:40:56Z
Created
2017-09-11T08:50:52Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr