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Related papers: Methanimine as a sink in the HCN and HNC solid sta…

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Experimental and theoretical studies are presented on the reactivity of the radical cation isomers methanimine and aminomethylene with ethyne. Selective isomer generation is performed via dissociative photoionization of suitable neutral…

We carried out an observational search for the recently discovered molecule H2NC, and its more stable isomer H2CN, toward eight cold dense clouds (L1544, L134N, TMC-2, Lupus-1A, L1489, TMC-1 NH3, L1498, and L1641N) and two diffuse clouds…

Astrophysics of Galaxies · Physics 2023-05-03 M. Agundez , O. Roncero , N. Marcelino , C. Cabezas , B. Tercero , J. Cernicharo

In this work, we present the results of our investigation into the chemistry of Z- and E-cyanomethanimine (HNCHCN), both of which are possible precursors to the nucleobase adenine. Ab initio quantum chemical calculations for a number of…

We report the first detection in the interstellar medium of $N$-cyanomethanimine (H$_2$CNCN), the stable dimer of HCN of highest energy, and the most complex organic molecule identified in space containing the prebiotically relevant NCN…

Context. Among the most significant chemical functional groups of interstellar molecules are the class of nitriles, which are proposed as key prebiotic molecules due to their chemical connection to the peptide bond after hydrolysis. CN…

Astrophysics of Galaxies · Physics 2025-07-16 Joan Enrique-Romero , Thanja Lamberts

The reaction between the amidogen, NH, radical and the ethyl, C2H5, radical has been investigated by performing electronic structure calculations of the underlying doublet potential energy surface. Rate coefficients and product branching…

Earth and Planetary Astrophysics · Physics 2018-10-25 Nadia Balucani , Dimitrios Skouteris , Cecilia Ceccarelli , Claudio Codella , Stefano Falcinelli , Marzio Rosi

Reactions occurring on the ice-covered surfaces of interstellar dust grains are considered to be among the most important sources of complex species in the interstellar medium. Despite this, molecules such as cyanamide, NH2CN, are largely…

Astrophysics of Galaxies · Physics 2026-04-20 Kevin M. Hickson , Jean-Christophe Loison , Audrey Coutens

We report the first detection in the interstellar medium of the Z-isomer of cyanomethanimine (HNCHCN), an HCN dimer proposed as precursor of adenine. We identified six transitions of Z-cyanomethanimine, along with five transitions of…

HCN is a molecule central to interstellar chemistry, since it is the simplest molecule containing a carbon-nitrogen bond and its solid state chemistry is rich. The aim of this work was to study the NH3 + HCN -> NH4+CN- thermal reaction in…

Earth and Planetary Astrophysics · Physics 2015-06-11 J. A. Noble , P. Theule , F. Borget , G. Danger , M. Chomat , F. Duvernay , F. Mispelaer , T. Chiavassa

Methane is typically thought to be formed in the solid state on the surface of cold interstellar icy grain mantles via the successive atomic hydrogenation of a carbon atom. In the current work we investigate the potential role of molecular…

Astrophysics of Galaxies · Physics 2022-04-06 Thanja Lamberts , Gleb Fedoseev , Marc van Hemert , Danna Qasim , Ko-Ju Chuang , Julia C. Santos , Harold Linnartz

A gas-phase formation route is proposed for the recently detected propargylimine molecule. In analogy to other imines, such as cyanomethanimine, the addition of a reactive radical (C$_2$H in the present case) to methanimine (CH$_2$NH})…

Astrophysics of Galaxies · Physics 2020-11-18 Jacopo Lupi , Cristina Puzzarini , Vincenzo Barone

HCN is among the most commonly detected molecules in star- and planet-forming regions. It is of broad interest as a tracer of star-formation physics, a probe of nitrogen astrochemistry, and an ingredient in prebiotic chemical schemes.…

Earth and Planetary Astrophysics · Physics 2022-07-27 Jennifer B. Bergner , Mahesh Rajappan , Karin I. Oberg

Recent studies of neutral gas-phase reactions characterized by barriers show that certain complex forming processes involving light atoms are enhanced by quantum mechanical tunneling at low temperature. Here, we performed kinetic…

Chemical Physics · Physics 2016-09-04 Kevin M. Hickson , Jean-Christophe Loison , Dianailys Nunez-Reyes , Raphael Mereau

Experimental and theoretical studies are presented on the reactivity of methanimine and aminomethylene cations with ethene. Selective isomer generation is performed via dissociative photoionization of suitable neutral precursors and…

The methaniminium cation, CH$_2$NH$_2^+$, plays an important role in Titan's N$_2$--CH$_4$ atmospheric chemistry. As the simplest protonated Schiff base (PSB), it also serves as a model for studying the nonadiabatic dynamics of retinal PSB,…

We conducted survey observations of a glycine precursor, methanimine or methylenimine (CH$_2$NH), with the NRO 45 m telescope and the SMT telescope towards 12 high-mass and two low-mass star-forming regions in order to increase number of…

Astrophysics of Galaxies · Physics 2016-07-13 Taiki Suzuki , Masatoshi Ohishi , Tomoya Hirota , Masao Saito , Liton Majumdar , Valentine Wakelam

Quantum chemical cluster calculations show that reactions of C$^+$ with HCN or HNC embedded in the surface of an icy grain mantle can account for the formation of a recently detected molecule, glycolonitrile, which is considered to be an…

Astrophysics of Galaxies · Physics 2021-01-13 David E. Woon

The hydrogen abstraction reaction between H and H$_2$S, yielding HS and H$_2$ as products, has been studied within the framework of interstellar surface chemistry. High-temperature rate constants up to 2000 K are calculated in the gas phase…

Astrophysics of Galaxies · Physics 2017-12-07 Thanja Lamberts , Johannes Kästner

Hydroxylamine (NH2OH) is one of the potential precursors of complex pre-biotic species in space. Here we present a detailed experimental study of hydroxylamine formation through nitric oxide (NO) surface hydrogenation for astronomically…

Astrophysics of Galaxies · Physics 2017-05-26 Gleb Fedoseev , Sergio Ioppolo , Thanja Lamberts , Junfeng Zhen , Herma M. Cuppen , Harold Linnartz

Context. In dense clouds, hydrogenation reactions on icy dust grains are key in the formation of molecules, like formaldehyde, methanol, and complex organic molecules (COMs). These species form through the sequential hydrogenation of CO…

Solar and Stellar Astrophysics · Physics 2018-09-28 K. -J. Chuang , G. Fedoseev , D. Qasim , S. Ioppolo , E. F. van Dishoeck , H. Linnartz
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