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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

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

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…

We report on the detection of hydromagnesium isocyanide, HMgNC, in the laboratory and in the carbon rich evolved star IRC+10216. The J=1-0 and J=2-1 lines were observed in our microwave laboratory equipment in Valladolid with a spectral…

Astrophysics of Galaxies · Physics 2015-06-17 Carlos Cabezas , Jose Cernicharo , Jose Luis Alonso , Marcelino Agundez , Santiago Mata , Michel Guelin , Isabel Peña

The pure rotational transitions of the protonated hydrogen cyanide ion, HCNH+, and its isotopic species, HCND+ and DCND+, were measured in the 107 - 482 GHz region with a source modulated microwave spectrometer. The ions were generated in…

Astrophysics · Physics 2009-10-30 M. Araki , H. Ozeki , S. Saito

Ethyl cyanide is an abundant molecule in hot molecular clouds. Lines from 13C isotopically substituted ethyl cyanide were identified in Orion. To enable the search and the possible detection of other isotopologues of ethyl cyanide in…

The reaction between carbon atoms and vinyl cyanide, CH2CHCN, is a formation route to interstellar 3-cyano propargyl radical, CH2C3N, a species that has recently been discovered in space. The 1-cyano propargyl radical (HC3HCN), an isomer of…

Astrophysics of Galaxies · Physics 2021-11-01 C. Cabezas , M. Nakajima , C. H. Chang , M. Agundez , Y. Endo , J. Cernicharo

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…

Among all closed-shell species observed in molecular clouds, molecules with C$_{3v}$ symmetry play a crucial role, as their rotational spectroscopy allows them to behave as a gas thermometer. In the interstellar medium, methyl cyanide…

Astrophysics of Galaxies · Physics 2023-09-22 M. Ben Khalifa , P. J. Dagdigian , J. Loreau

Sulfur-bearing molecules are central to interstellar chemistry, yet their observed abundances in the gas phase remain far below cosmic expectations in dense interstellar regions. Mixed N-S-O species such as thionylimide (HNSO) are…

Astrophysics of Galaxies · Physics 2025-12-01 Valerio Lattanzi , Miguel Sanz-Novo , Víctor M. Rivilla , Izaskun Jiménez-Serra , Paola Caselli

HC$_3$N is an ubiquitous molecule in interstellar environments, from external galaxies, to Galactic interstellar clouds, star forming regions, and planetary atmospheres. Observations of its rotational and vibrational transitions provide…

We report the first identification in space of HC$_3$N$^+$, the simplest member of the family of cyanopolyyne cations. Three rotational transitions with half-integer quantum numbers from $J$=7/2 to 11/2 have been observed with the Yebes 40m…

Astrophysics of Galaxies · Physics 2024-07-03 C. Cabezas , M. Agúndez , Y. Endo , B. Tercero , N. Marcelino , P. de Vicente , J. Cernicharo

Very recently, molecular rotational transitions observed in the photon-dominated region of the Horsehead nebula have been attributed to l-C3H+. In an effort to corroborate this finding, we employed state-of-the art and proven high-accuracy…

High Energy Astrophysical Phenomena · Physics 2013-05-09 Xinchuan Huang , Ryan C. Fortenberry , Timothy J. Lee

Rotational transitions of $iso$-propyl cyanide, (CH$_3$)$_2$CHCN, also known as $iso$-butyronitrile, were recorded using long-path absorption spectroscopy in selected regions between 37 and 600 GHz. Further measurements were carried out…

Instrumentation and Methods for Astrophysics · Physics 2019-03-21 Holger S. P. Müller , Audrey Coutens , Adam Walters , Jens-Uwe Grabow , Stephan Schlemmer

This work provides the first full set of vibrational and rotational spectral data needed to aid in the detection of AlH$_3$OH$_2$, SiH$_3$OH, and SiH$_3$NH$_2$ in astrophysical or simulated laboratory environments through the use of quantum…

Instrumentation and Methods for Astrophysics · Physics 2021-09-27 A. G. Watrous , B. R. Westbrook , M. C. Davis , Ryan C. Fortenberry

We report the first laboratory and interstellar detection of the alpha-cyano vinyl radical (H2CCCN). This species was produced in the laboratory by an electric discharge of a gas mixture of vinyl cyanide, CH2CHCN, and Ne, and its rotational…

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…

Among the numerous molecular systems found in the interstellar medium (ISM), vinyl cyanide is the first identified olephinic nitrile. While it has been observed in various sources, its detection in Sgr B2 is notable as the 2$_{11}$-2$_{12}$…

Astrophysics of Galaxies · Physics 2025-06-23 Karina Sogomonyan , Malek Ben Khalifa , Jérôme Loreau

C-cyanomethanimine (HNCHCN), existing in the two $Z$ and $E$ isomeric forms, is a key prebiotic molecule, but, so far, only the $E$ isomer has been detected toward the massive star-forming region. Sagittarius B2(N) using transitions in the…

The C-star envelope IRC+10216 harbors a rich variety of molecules, with more than 80 detected to date. During the course of a $\lambda$ 3 mm survey of IRC+10216 carried out with the IRAM 30-m telescope we have detected various weak lines,…

Astrophysics of Galaxies · Physics 2014-10-15 Marcelino Agúndez , José Cernicharo , Michel Guélin
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