Abstract

Context. The spectra of four low-lying vibrational states of both anti and gauche conformers of normal-propyl cyanide were previously measured and analyzed in two spectral windows between 36 and 127 GHz. All states were then identified in a spectral line survey called Exploring Molecular Complexity with ALMA (EMoCA) toward Sagittarius B2(N) between 84.1 and 114.4 GHz with the Atacama Large Millimeter/submillimeter Array (ALMA) in its Cycles 0 and 1. Aims. We wanted to extend the measurements and analysis up to 506 GHz to provide accurate predictions over a much wider range of frequencies, quantum numbers and energies. Methods. We carried out measurements in two additional frequency windows up to 506 GHz. Results. For the gauche conformer, a large number of both a- and b-type transitions were identified. For the anti conformer, transitions were predominantly, but not exclusively, a-type. We hence improved molecular parameters for the ground states of both anti- and gauche-n-propyl cyanide and for excited vibrational states of the gauche conformer (v30 = 1, v29 = 1, v30 = 2, v28 = 1) and anti conformer (v30 = 1, v18 = 1, v30 = 2, v29 = 1) with high order coupling parameters determined between v18 = 1 and v30 = 2. Parameters are published for the first time for v18 = v30 = 1 of the anti conformer and for v29 = v30 = 1 of the gauche conformer. Conclusions. In total 15385 lines have been incorporated in the fits and should allow good predictions for unperturbed lines over the whole operating range of radio-telescopes. Evidence is found for vibrational coupling for some levels above 380 GHz. The coupling between v18 = 1 and v30 = 2 of the anti conformer has been well characterized. An additional list of 740 lines showing potential but as yet unidentified coupling has been provided for astrophysical identification.

Highlights

  • Molecules in vibrationally excited states are generally found in hot dense and possibly shocked regions of space and can be used as probes of the gas close to deeply embedded luminous infrared sources

  • The present data should be useful to search for vibrationally excited states of n-PrCN in Orion KL where transitions of the ground vibrational states of both conformers were detected recently with Atacama Large Millimeter/submillimeter Array (ALMA) (Pagani et al 2017)

  • During our work we extended the spectral analysis of the ground state, and carried out new work on the combination states of v18 = v30 = 1 for the anti conformer and v29 = v30 = 1 for the gauche conformer

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Summary

Introduction

Molecules in vibrationally excited states are generally found in hot dense and possibly shocked regions of space and can be used as probes of the gas close to deeply embedded luminous infrared sources. The laboratory spectroscopic study up to 127 GHz of these vibrationally excited states (Müller et al 2016) led to their detection in space as explained above Following this identification we decided to carry out a more extensive analysis up to 506 GHz of these vibrational states with the aim of providing reliable predictions over the whole operating band of ALMA. The present data should be useful to search for vibrationally excited states of n-PrCN in Orion KL where transitions of the ground vibrational states of both conformers were detected recently with ALMA (Pagani et al 2017). During our work we extended the spectral analysis of the ground state, and carried out new work on the combination states of v18 = v30 = 1 for the anti conformer and v29 = v30 = 1 for the gauche conformer Transitions of these and other higher-lying vibrational states may be observable in the new EMoCA data obtained in ALMA Cycle 4

Laboratory spectroscopic details
Ground vibrational state
Conclusion and outlook

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