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The rotational spectrum of the formaldehyde isotopologue H$_2$C$^{17}$O was investigated between 0.56 and 1.50 THz using a sample of natural isotopic composition. In addition, transition frequencies were determined for H$_2$C$^{18}$O and…

Astrophysics of Galaxies · Physics 2019-03-13 Holger S. P. Müller , Frank Lewen

The rotational spectra of thioisocyanic acid (HNCS), and its three energetic isomers (HSCN, HCNS, and HSNC) have been observed at high spectral resolution by a combination of chirped-pulse and Fabry-P\'{e}rot Fourier-transform microwave…

An investigation of the rotational spectrum of the interstellar molecule thioformaldehyde between 110 and 377 GHz through a pyrolysis reaction revealed a multitude of absorption lines assignable to H$_2$CS and H$_2$C$^{34}$S in their lowest…

Cyclopropenone was first detected in the cold and less dense envelope of Sagittarius B2(N). It was found later in several cold dark clouds and it may be possible to detect its minor isotopic species in these environments. In addition, the…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 Holger S. P. Müller , Ananya Brahmi M. , Jean-Claude Guillemin , Frank Lewen , Stephan Schlemmer

Thioformamide NH2CHS is a sulfur-bearing analog of formamide NH2CHO. The latter was detected in the interstellar medium back in the 1970s. Most of the sulfur-containing molecules detected in the interstellar medium are analogs of…

Astrophysics of Galaxies · Physics 2021-09-08 R. A. Motiyenko , A. Belloche , R. T. Garrod , L. Margulès , H. S. P. Müller , K. M. Menten , J. -C. Guillemin

A better understanding of sulphur chemistry is needed to solve the interstellar sulphur depletion problem. A way to achieve this goal is to study new S-bearing molecules in the laboratory, obtaining accurate rest frequencies for an…

Astrophysics of Galaxies · Physics 2018-04-25 D. Prudenzano , J. Laas , L. Bizzocchi , V. Lattanzi , C. Endres , B. M. Giuliano , S. Spezzano , M. E. Palumbo , P. Caselli

Using arguments parallel to those used in support of using H2CO as a sensitive probe of temperature and density in molecular clouds, we measured the J=7-6 and J=10-9 transitions of thioformaldehyde (H2CS) in several hot core sources. The…

Astrophysics of Galaxies · Physics 2009-07-24 Alwyn Wootten , Jeffrey G. Mangum

Submillimeter spectra of three isotopomers of propyne containing one $^{13}$C atom were recorded in natural isotopic composition in the region of 426 GHz to 785 GHz. Additional measurements were carried out near 110 GHz. Combining these…

Instrumentation and Methods for Astrophysics · Physics 2020-02-03 Holger S. P. Müller , Sven Thorwirth , Frank Lewen

We present observations of the singly and doubly deuterated species of thioformaldehyde, HDCS and D$_2$CS, towards the dark cloud Barnard 1. This is the first detection of D$_2$CS in Space and in dense and cold prestellar regions. Column…

Astrophysics · Physics 2009-11-10 N. Marcelino , J. Cernicharo , E. Roueff , M. Gerin , R. Mauersberger

We report the gas-phase detection and spectroscopic characterization of ethynethiol ($\mathrm{HCCSH}$), a metastable isomer of thioketene ($\mathrm{H_2C_2S}$) using a combination of Fourier-transform microwave and submillimeter-wave…

The rotational spectra of singly substituted $^{13}$C and $^{15}$N isotopic species of vinyl cyanide have been studied in natural abundances between 64 and 351 GHz. In combination with previous results, greatly improved spectroscopic…

Methyl cyanide is an important trace molecule in star-forming regions. It is one of the more common molecules used to derive kinetic temperatures in such sources. As preparatory work for Herschel, SOFIA, and in particular ALMA we want to…

Astrophysics of Galaxies · Physics 2019-03-21 Holger S. P. Müller , Brian J. Drouin , John C. Pearson

Protonated molecular species have been proven to be abundant in the interstellar gas. This class of molecules is also pivotal for the determination of important physical parameters for the ISM evolution (e.g. gas ionisation fraction) or as…

The rotational spectrum of the most stable conformer of ethylene glycol (HO(CH$_2$)$_2$OH) has been recorded between 360-890 GHz using a frequency-modulation sub-millimeter spectrometer. The refinement and extension of the spectroscopic…

Astrophysics of Galaxies · Physics 2020-07-01 Mattia Melosso , Luca Dore , Filippo Tamassia , Crystal L. Brogan , Todd R. Hunter , Brett A. McGuire

This work aims to spectroscopically characterize and provide for the first time direct experimental frequencies of the ground vibrational state and two excited states of the simplest alkynyl thiocyanate (HCCSCN) for astrophysical use. Both…

Cyanoformaldehyde (HCOCN) molecule has recently been suspected towards the Sagittarius B2(N) by the Green Bank telescope, though a confirmation of this observation has not yet been made. In and around a star forming region, this molecule…

Astrophysics of Galaxies · Physics 2015-06-16 Ankan Das , Liton Majumdar , Sandip K. Chakrabarti , Rajdeep Saha , Sonali Chakrabarti

Methyl cyanide is an important trace molecule in space, especially in star-forming regions where it is one of the more common molecules used to derive kinetic temperatures. We want to obtain accurate spectroscopic parameters of minor…

Astrophysics of Galaxies · Physics 2019-03-21 H. S. P. Müller , B. J. Drouin , J. C. Pearson , M. H. Ordu , N. Wehres , F. Lewen

Thioacetamide (CH3CSNH2) is the sulfur analog to acetamide (CH3CONH2) and it is a viable candidate to search for in astronomical environments specifically toward regions where other S-bearing molecules have been found and, if possible, that…

Using reflective cross-polarized 2D THz time-domain spectroscopy in the range of 1-12 THz, we follow the trajectory of the out-of-equilibrium electron population in the low-bandgap semiconductor InSb. The 2D THz spectra show a set of…

Strongly Correlated Electrons · Physics 2019-06-10 S. Houver , L. Huber , M. Savoini , E. Abreu , S. L. Johnson

The study of the rotational spectrum of NaCN (X $^1$A') has recently been extended in frequency and in quantum numbers. Difficulties have been encountered in fitting the transition frequencies within experimental uncertainties. Various…

Astrophysics of Galaxies · Physics 2019-03-13 Holger S. P. Müller , D. T. Halfen , L. M. Ziurys
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