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AIM: We have recently developed a microscopic Monte Carlo approach to study surface chemistry on interstellar grains and the morphology of ice mantles. The method is designed to eliminate the problems inherent in the rate-equation formalism…

天体物理学 · 物理学 2009-11-13 Q. Chang , H. M. Cuppen , E. Herbst

Small imines containing up to three carbon atoms are present in the interstellar medium. As alkynyl compounds are abundant in this medium, propargylimine thus represents a promising candidate for a new interstellar detection. The goal of…

We report the discovery of propylene (also called propene, CH_2CHCH_3) with the IRAM 30-m radio telescope toward the dark cloud TMC-1. Propylene is the most saturated hydrocarbon ever detected in space through radio astronomical techniques.…

天体物理学 · 物理学 2009-11-13 N. Marcelino , J. Cernicharo , M. Agundez , E. Roueff , M. Gerin , J. Martin-Pintado , R. Mauersberger , C. Thum

We have performed reaction product screening measurements using broadband rotational spectroscopy to identify rotational transition matches between laboratory spectra and the Green Bank Telescope PRIMOS radio astronomy survey spectra in…

Cold cores are an early step of star formation, characterized by densities > 10$^4$ cm$^{-3}$, low temperatures (< 15 K), and very low external UV radiation. We investigate the physico-chemical processes at play to tracing the origin of…

星系天体物理 · 物理学 2023-01-04 A. Taillard , V. WakelaM , P. Gratier , E. Dartois , M. Chabot , J. A. Noble , J. V. Keane , A. C. A. Boogert , D. Harsono

(Abridged) We aim to enlarge the number of known hot corinos and carry out a first comparative study with hot cores. The ultimate goal is to understand whether complex organic molecules form in the gas phase or on grain surfaces, and what…

天体物理学 · 物理学 2015-06-24 Sandrine Bottinelli , Cecilia Ceccarelli , Jonathan P. Williams , Bertrand Lefloch

In this paper we use observations of molecular tracers in metal rich and alpha-enhanced galaxies to study the effect of abundance changes on molecular chemistry. We selected a sample of metal rich spiral and star bursting objects from the…

宇宙学与河外天体物理 · 物理学 2015-06-15 Timothy A. Davis , Estelle Bayet , Alison Crocker , Selcuk Topal , Martin Bureau

The presence of carbon-chain molecules in the interstellar medium (ISM) has been known since the early 1970s and $>130$ such species have been identified to date, making up $\sim 43$% of the total of detected ISM molecules. They are…

星系天体物理 · 物理学 2024-04-15 Kotomi Taniguchi , Prasanta Gorai , Jonathan C. Tan

We present strong detections of methyl cyanide, vinyl cyanide, ethyl cyanide and cyanodiacetylene molecules with the Green Bank Telescope (GBT) toward the Sgr B2(N) molecular cloud. Attempts to detect the corresponding isocyanide isomers…

天体物理学 · 物理学 2009-11-13 Anthony J. Remijan , J. M. Hollis , F. J. Lovas , D. F. Plusquellic , P. R. Jewell

Based on a novel laboratory method, 14 mm-wave lines of the molecular ion H$_2$CCCH$^+$ have been measured in high resolution, and the spectroscopic constants of this asymmetric rotor determined with high accuracy. Using the Yebes 40 m and…

The detection of the amino acid glycine and its amine precursor methylamine on the comet 67P/Churyumov-Gerasimenko by the Rosetta mission provides strong evidence for a cosmic origin of prebiotics on Earth. How and when such complex organic…

天体物理仪器与方法 · 物理学 2020-11-17 S. Ioppolo , G. Fedoseev , K. -J. Chuang , H. M. Cuppen , A. R. Clements , M. Jin , R. T. Garrod , D. Qasim , V. Kofman , E. F. van Dishoeck , H. Linnartz

HCN molecules serve as an important tracer for chemical evolution of elemental nitrogen in the regions of star and planet formation. This is largely explained by the fact that N atoms and N$_2$ molecules are poorly accessible for the…

Observations are presented of emission lines from organic molecules at frequencies 32 - 50 GHz in the vicinity of Chamaeleon MMS1. This chemically-rich dense cloud core habours an extremely young, very low-luminosity protostellar object and…

星系天体物理 · 物理学 2015-05-30 Martin A. Cordiner , Steven B. Charnley , Eva S. Wirström , Robert G. Smith

We report the detection for the first time in space of three new pure hydrocarbon cycles in TMC-1: c-C3HCCH (ethynyl cyclopropenylidene), c-C5H6 (cyclopentadiene) and c-C9H8 (indene). We derive a column density of 3.1e11 cm-2 for the former…

星系天体物理 · 物理学 2021-05-19 J. Cernicharo , M. Agundez , C. Cabezas , B. Tercero , N. Marcelino , J. R. Pardo , P. de Vicente

We report the detection, for the first time in space, of cyano thioformaldehyde (HCSCN) and propynethial (HCSCCH) towards the starless core TMC-1. Cyano thioformaldehyde presents a series of prominent a- and b-type lines, which are the…

星系天体物理 · 物理学 2021-06-23 J. Cernicharo , C. Cabezas , Y. Endo , M. Agundez , B. Tercero , J. R. Pardo , N. Marcelino , P. de Vicente

Hexamethylentetramine has drawn a lot of attention due to its potential to produce prebiotic species. This work aims to gain a better understanding in the chemical processes concerning methylamine under astrophysically relevant conditions.…

天体物理仪器与方法 · 物理学 2021-07-14 H. Carrascosa , C. González Díaz , G. M. Muñoz Caro , P. C. Gómez , M. L. Sanz

Benzonitrile (c-C6H5CN) has been recently detected in cold and dense regions of the interstellar medium (ISM), where it has been used as a signpost of a rich aromatic organic chemistry that might lead to the production of polycyclic…

We report the detection of the oxygen-bearing complex organic molecules propenal (C2H3CHO), vinyl alcohol (C2H3OH), methyl formate (HCOOCH3), and dimethyl ether (CH3OCH3) toward the cyanopolyyne peak of the starless core TMC-1. These…

星系天体物理 · 物理学 2021-05-05 M. Agundez , N. Marcelino , B. Tercero , C. Cabezas , P. de Vicente , J. Cernicharo

GEMS is an IRAM 30m Large Program whose aim is determining the elemental depletions and the ionization fraction in a set of prototypical star-forming regions. This paper presents the first results from the prototypical dark cloud TMC 1.…

This is the first in a series of three papers describing a project with the Cosmic Origins Spectrograph on the Hubble Space Telescope to measure abundances of the neutral interstellar medium (ISM) in a sample of 9 nearby star-forming…

星系天体物理 · 物理学 2015-06-22 Bethan L. James , Alessandra Aloisi , Timothy M. Heckman , Sangmo Tony Sohn , Michael A. Wolfe