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相关论文: Discovery of the Interstellar Chiral Molecule Prop…

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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

The recent identification of the first complex chiral molecule, propylene oxide (PrO) in space opens up a new window to further study the origin of homochirality on the Earth. There are some recent studies to explain the formation of PrO…

太阳与恒星天体物理 · 物理学 2019-08-14 Ankan Das , Prasanta Gorai , Sandip K. Chakrabarti

(Abridged) Life is distinctly homochiral. The origins of this homochirality are under active debate. Recently, propylene-oxide has been detected in the gas-phase interstellar medium (ISM) (McGuire et al. 2016). The enantiomeric composition…

星系天体物理 · 物理学 2022-10-19 Boy Lankhaar

The first set of theoretical cross sections for propylene oxide (CH3CHCH2O) colliding with cold He atoms has been obtained at the full quantum level using a high-accuracy potential energy surface. By scaling the collision reduced mass,…

Human biology has a preference for left-handed chiral molecules and an outstanding question is if this is imposed through astrophysical origins. We aim to evaluate the known information about chiral molecules within astrophysical and…

天体物理仪器与方法 · 物理学 2024-01-19 Chenoa D. Tremblay , Roger D. Amos , Rika Kobayashi

Complex organic molecules, such as propylene (CH3CHCH2), are detected in molecular clouds (such as TMC1) with high fractional abundances (~2.10^{-9}, relative to hydrogen) that cannot be explained by gas-phase chemical reactions under…

星系天体物理 · 物理学 2015-06-16 J. M. C. Rawlings , D. A. Williams , S. Viti , C. Cecchi-Pestellini

The chemical compounds carrying the thiol group (-SH) have been considered essential in recent prebiotic studies regarding the polymerization of amino acids. We have searched for this kind of compounds toward the Galactic Centre quiescent…

We present a clear detection of CH2 in absorption towards the molecular cloud complexes Sagittarius B2 and W49 N using the ISO Long Wavelength Spectrometer. These observations represent the first detection of its low excitation rotational…

天体物理学 · 物理学 2009-11-10 E. T. Polehampton , K. M. Menten , S. Bruenken , G. Winnewisser , J. -P. Baluteau

Propylene oxide, a favorite target of experimental and theoretical studies of circular dichroism, was recently discovered in interstellar space, further amplifying the attention to its role in the current debate on protobiological…

Intimately connected to the rule of life, chirality remains a long-time fascination in biology, chemistry, physics and materials science. Chiral structures, e.g., nucleic acid and cholesteric phase developed from chiral molecules are common…

The tentative detection of 3-hydroxypropanal (HO(CH$_2$)$_2$C(O)H) toward the Galactic center molecular cloud G+0.693-0.027 prompts a systematic survey in this source aimed at detecting all C$_3$H$_6$O$_2$ isomers with available…

The detection of complex organic molecules (COMs) toward dense, collapsing prestellar cores has sparked interest in the fields of astrochemistry and astrobiology, yet the mechanisms for COM formation are still debated. It was originally…

星系天体物理 · 物理学 2023-04-05 Samantha Scibelli , Yancy Shirley

Context. Propyne (CH$_3$CCH) has been detected in a variety of environments, from Galactic star-forming regions to extragalactic sources. Such molecules are excellent tracers of the physical conditions in star-forming regions. Aims. This…

Complex organic molecules with three carbon atoms are found in the earliest stages of star formation. In particular, propenal (C$_2$H$_3$CHO) is a species of interest due to its implication in the formation of more complex species and even…

Characterizing the molecular composition of solar-type protostars is useful for improving our understanding of the physico-chemical conditions under which the Sun and its planets formed. In this work, we analyzed the Atacama Large…

星系天体物理 · 物理学 2022-04-20 A. Coutens , J. -C. Loison , A. Boulanger , E. Caux , H. S. P. Müller , V. Wakelam , S. Manigand , J. K. Jørgensen

Observations with the Short Wavelength Spectrometer (SWS) onboard the {\it Infrared Space Observatory} (ISO) have led to the first detection of the methyl radical ${\rm CH_3}$ in the interstellar medium. The $\nu_2$ $Q-$branch at 16.5…

天体物理学 · 物理学 2009-10-31 H. Feuchtgruber , F. P. Helmich , E. F. van Dishoeck , C. M. Wright

The molecular species hydrogen peroxide, HOOH, is likely to be a key ingredient in the oxygen and water chemistry in the interstellar medium. Our aim with this investigation is to determine how abundant HOOH is in the cloud core {\rho} Oph…

星系天体物理 · 物理学 2011-06-02 P. Bergman , B. Parise , R. Liseau , B. Larsson , H. Olofsson , K. M. Menten , R. Güsten

One of the open questions in astrochemistry is how complex organic and prebiotic molecules are formed. Aims. Our aim is to start the process of compiling an inventory of oxygen-bearing complex organic molecules toward the solar-type Class 0…

In recent years, organic molecules of increasing complexity have been found toward the prolific Galactic center source Sagittarius B2. We wish to explore the degree of complexity that the interstellar chemistry can reach in star-forming…

星系天体物理 · 物理学 2014-08-25 A. Belloche , R. T. Garrod , H. S. P. Müller , K. M. Menten , C. Comito , P. Schilke

(abridged) We review recent studies of chirality using circularly polarized light, along with the birth and evolution of life and planetary systems. Terrestrial life consists almost exclusively of one enantiomer, left-handed amino acids.…

星系天体物理 · 物理学 2011-12-08 Tsubasa Fukue
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