Detection of a New Molecular Ion HC 3NH + in TMC-1
Abstract
Protonated cyanoacetylene HC3NH(+) has been detected toward TMC-1 for the first time with the Nobeyama 45 m radiotelescope through the J = 5-4 and J = 4-3 transitions. This observation provides the first measurement of the pure rotational transitions for this ion either in the laboratory or in space. From a simultaneous analysis of rotational transition frequencies obtained in this work and the previous infrared data, the most accurate rotational and the centrifugal distortion constants were determined to be B = 4329.0047(10) and D = 0.000478(11) MHz, respectively, with one standard deviation in parentheses. The column density of HC3NH(+) in TMC-1 (cyanopolyyne peak) was determined to be 1.0 (0.2) x 1012/sq cm which is 160 times smaller than that of HC3N and 2.6 times more abundant than HNCCC. The abundances of HC3NH(+), HNCCC, and HCCCN are discussed on the basis of a reaction mechanism recently proposed for the production of HCCCN through neutral-neutral reactions.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 1994
- DOI:
- 10.1086/187171
- Bibcode:
- 1994ApJ...420L..95K
- Keywords:
-
- Cyanoacetylene;
- Dark Matter;
- Doppler-Fizeau Effect;
- Microwave Spectra;
- Molecular Clouds;
- Radio Astronomy;
- Radio Spectra;
- Spectroscopy;
- Atmospheric Density;
- Chemical Reactions;
- Radio Telescopes;
- Spectrometers;
- Temperature;
- Astronomy;
- ISM: ABUNDANCES;
- ISM: INDIVIDUAL ALPHANUMERIC: TMC-1;
- LINE: IDENTIFICATION;
- MOLECULAR DATA;
- RADIO LINES: ISM