Abstract
The pure rotational spectrum of the CaCCH radical (X2Σ+) has been measured in the laboratory using millimeter/submillimeter direct absorption spectroscopy. The species was created in a d.c. discharge by the reaction of calcium vapor and acetylene. Twenty-two rotational transitions of this molecule were recorded in the frequency range 230-380 GHz to an accuracy of ± 150 kHz. Spin-rotation splittings, but no proton hyperfine structure, were observed for CaCCH. The data were analyzed using a 2Σ Hamiltonian, and rotational and fine structure constants were determined. These measurements have resulted in accurate rest frequencies for CaCCH to be used for astronomical searches. A calcium-bearing molecule has yet to be observed in interstellar or circumstellar gas.
| Original language | English (US) |
|---|---|
| Pages (from-to) | L57-L60 |
| Journal | Astrophysical Journal |
| Volume | 444 |
| Issue number | 1 PART 2 |
| DOIs | |
| State | Published - May 1 1995 |
Keywords
- ISM: molecules
- Line: identification
- Molecular data
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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