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相关论文: Reactions of Acetonitrile with Trapped, Translatio…

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The gas-phase reaction of CCl+ with acetonitrile (CH3CN) is studied using a linear Paul ion trap coupled to a time-of-flight mass spectrometer. This work builds on a previous study of the reaction of CCl+ with acetylene and further explores…

Ion-neutral chemical reactions are important in several areas of chemistry, including in some regions of the interstellar medium, planetary atmospheres, and comets. Reactions of CCl+ with C2H2 are measured and the main products include…

The product formation channels of ground state carbon atoms, C(3P), reacting with ammonia, NH3, have been investigated using two complementary experiments and electronic structure calculations. Reaction products are detected in a gas flow…

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…

地球与行星天体物理 · 物理学 2018-10-25 Nadia Balucani , Dimitrios Skouteris , Cecilia Ceccarelli , Claudio Codella , Stefano Falcinelli , Marzio Rosi

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…

星系天体物理 · 物理学 2025-07-16 Joan Enrique-Romero , Thanja Lamberts

The reactions of ground state atomic carbon, C(3P), are likely to be important in astrochemistry due to the high abundance levels of these atoms in the dense interstellar medium. Here we present a study of the gas-phase reaction between…

星系天体物理 · 物理学 2023-09-15 Kevin M. Hickson , Jean-Christophe Loison , Valentine Wakelam

Rate constants have been measured for the C(3P) + CH3CN reaction between 50 K and 296 K using a continuous-flow supersonic reactor. C(3P) atoms were created by the in-situ pulsed laser photolysis of CBr4 at 266 nm, while the kinetics of…

星系天体物理 · 物理学 2021-03-26 Kevin M. Hickson , Jean-Christophe Loison , Valentine Wakelam

Oxygen atom addition and insertion reactions may provide a pathway to chemical complexity in ices that are too cold for radicals to diffuse and react. We have studied the ice-phase reactions of photo-produced oxygen atoms with C2…

地球与行星天体物理 · 物理学 2019-04-03 Jennifer B. Bergner , Karin I. Oberg , Mahesh Rajappan

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…

Rate constants for the C(3P) + CH3OH reaction have been measured in a continuous supersonic flow reactor over the range 50 K to 296 K. C(3P) was created by the in-situ pulsed laser photolysis of CBr4, a multiphoton process which also…

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…

星系天体物理 · 物理学 2021-01-13 David E. Woon

Aminoacetonitrile (AAN), also known as glycinenitrile, has been suggested as a possible precursor of glycine and adenine in the interstellar medium. Here we present the chemical modeling of AAN and its isomers in hot cores using the…

星系天体物理 · 物理学 2024-08-22 Xia Zhang , Donghui Quan , Xiaohu Li , Jarken Esimbek , Fangfang Li , Yan Zhou , Dalei Li

Reactions involving atomic carbon in its ground electronic state, C(3P), play an important role in astrochemistry due to high C-atom abundance levels. Here we performed a kinetic investigation of the reaction between C(3P) and acetaldehyde,…

星系天体物理 · 物理学 2025-06-06 Kevin M. Hickson , Jean-Christophe Loison , Valentine Wakelam

We report the first interstellar identification of protonated acetylene, C2H3+, a fundamental hydrocarbon, in the z=0.89 molecular absorber toward the gravitationally lensed quasar PKS1830-211. The molecular species is identified from clear…

星系天体物理 · 物理学 2024-01-19 S. Muller , R. Le Gal , E. Roueff , J. H. Black , A. Faure , M. Guelin , A. Omont , M. Gerin , F. Combes , S. Aalto

Atomic carbon in its ground electronic state, C(3P), is expected to be present at high abundances during the evolution of dense molecular clouds. Consequently, its reactions with other interstellar species could have a strong influence on…

星系天体物理 · 物理学 2024-05-03 Kevin M. Hickson , Jean-Christophe Loison , Valentine Wakelam

Cyclopentadiene (c-C5H6) is considered a key molecule in the formation of polycyclic aromatic hydrocarbons (PAHs) in the interstellar medium (ISM). The synthesis of PAHs from simpler precursors is known as the "bottom-up" theory, which, so…

We report the first detection in interstellar space of the 3-cyano propargyl radical (CH2C3N). This species was observed in the cold dark cloud TMC-1 using the Yebes 40m telescope. A total of seven rotational transitions for both ortho- and…

We sought to determine which are the main hydrogenation paths of acetaldehyde (CH3CHO). As a partially unsaturated molecule, CH3CHO can have links with more hydrogenated species, like ethanol (C2H5OH) or with more unsaturated ones, like…

星系天体物理 · 物理学 2025-02-26 Germán Molpeceres , Thanh Nguyen , Yasuhiro Oba , Naoki Watanabe

Using the Yebes 40m and IRAM 30m radiotelescopes, we detected two series of harmonically related lines in space that can be fitted to a symmetric rotor. The lines have been seen towards the cold dense cores TMC-1, L483, L1527, and L1544.…

The chemistry of planetary atmospheres containing molecular nitrogen as a major atmospheric component is strongly influenced by the reactions of atomic nitrogen. Although nitrogen atoms in their ground electronic state N(4S) are mostly…

地球与行星天体物理 · 物理学 2025-11-11 Kevin M. Hickson , Jean-Christophe Loison , Benjamin Benne , Michel Dobrijevic
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