Issue |
A&A
Volume 464, Number 3, March IV 2007
|
|
---|---|---|
Page(s) | L33 - L36 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20066964 | |
Published online | 05 February 2007 |
Letter to the Editor
Laboratory detection of the negative molecular ion CCH-
1
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA, and Division of Engineering and Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138, USA e-mail: sbruenken@cfa.harvard.edu
2
Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, The University of Texas, Austin, TX 78712, USA
Received:
19
December
2006
Accepted:
19
January
2007
Aims.This paper reports the laboratory detection of the rotational spectrum of the acetylide anion, CCH-.
Methods.Five successive rotational transitions have been measured to high accuracy in a dc discharge with a free space millimeter-wave spectrometer in the frequency range 83–417 GHz.
Results.Precise spectroscopic constants have been obtained for CCH- and transition rest frequencies can now be calculated to better than 1 km s-1 in equivalent radial velocity far into the terahertz region, allowing for deep astronomical searches for this anion in space. The highly stable and fairly polar CCH- anion is a likely candidate for radio astronomical detection, its neutral analogue CCH being among one of the most abundant molecules in a wide variety of astrophysical sources.
Key words: line: identification / molecular data / astrochemistry / methods: laboratory / ISM: molecules / radio lines: ISM
© ESO, 2007
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