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相关论文: First detection of doubly deuterated methyl acetyl…

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The abundances of deuterated molecules with respect to their main isotopologue counterparts have been determined to be orders of magnitude higher than expected from the cosmic abundance of deuterium relative to hydrogen. The increasing…

星系天体物理 · 物理学 2023-03-01 J. Ferrer Asensio , S. Spezzano , L. H. Coudert , V. Lattanzi , C. P. Endres , J. K. Jørgensen , P. Caselli

We report the first detection in space of the single deuterated isotopologue of methyldiacetylene, CH2DC4H. A total of 12 rotational transitions, with J = 8-12 and Ka = 0 and 1, were identified for this species in TMC-1 in the 31.0-50.4 GHz…

星系天体物理 · 物理学 2022-01-12 C. Cabezas , R. Fuentetaja , E. Roueff , M. Agundez , B. Tercero , N. Marcelino , J. R. Pardo , P. de Vicente , J. Cernicharo

We report the first detection in space of the single deuterated isotopologue of methylcyanoacetylene, CH$_2$DC$_3$N. A total of fifteen rotational transitions, with $J$ = 8-12 and $K_a$ = 0 and 1, were identified for this species in TMC-1…

星系天体物理 · 物理学 2021-06-23 C. Cabezas , E. Roueff , B. Tercero , M. Agúndez , N. Marcelino , P. de Vicente , J. Cernicharo

Studies of deuterated isotopologues of complex organic molecules can provide important constraints on their origin in regions of star formation. In particular, the abundances of deuterated species are very sensitive to the physical…

Methyl acetate (CH_3COOCH_3) has been recently observed by IRAM 30 m radio telescope in Orion though the presence of its deuterated isotopomers is yet to be confirmed. We therefore study the properties of various forms of methyl acetate,…

星系天体物理 · 物理学 2015-08-06 Ankan Das , Liton Majumdar , Dipen Sahu , Prasanta Gorai , B Sivaraman , Sandip K. Chakrabarti

We report the first detection of doubly-deuterated methanol (CHD2OH), as well as firm detections of the two singly-deuterated isotopomers of methanol (CH2DOH and CH3OD), towards the solar-type protostar IRAS16293-2422. From the present…

High deuterium fractionation is observed in various types of environment such as prestellar cores, hot cores and hot corinos. It has proven to be an efficient probe to study the physical and chemical conditions of these environments. The…

Using the IRAM 30m telescope, we mapped the methanol emission in the pre-stellar core L1544 and observed singly deuterated methanol (CH$_2$DOH and CH$_3$OD) towards the dust peak of L1544. Non-LTE radiative transfer modelling was performed…

太阳与恒星天体物理 · 物理学 2014-09-17 Luca Bizzocchi , Paola Caselli , Silvia Spezzano , Elvira Leonardo

We report the first interstellar detection of c-C3D2. The doubly deuterated cyclopropenylidene, a carbene, has been detected toward the starless cores TMC- 1C and L1544 using the IRAM 30m telescope. The J(Ka,Kc) = 3(0,3)-2(1,2),…

We have started a measurement campaign of numerous methanol isotopologs in low-lying torsional states in order to provide extensive line lists for radio astronomical observations from an adequate spectroscopic model and to investigate how…

The isotopic ratios of deuterated methanol derived around protostars are commonly used to infer the physical conditions under which they formed in the earlier prestellar stage. However, there is a discrepancy in the ratio of the singly…

We report the first detection of triply-deuterated methanol, with 12 observed transitions, towards the low-mass protostar IRAS 16293-2422, as well as multifrequency observations of 13CH3OH, used to derive the column density of the main…

天体物理学 · 物理学 2007-05-23 B. Parise , A. Castets , E. Herbst , E. Caux , C. Ceccarelli , I. Mukhopadhyay , A. G. G. M. Tielens

The inheritance of material across the star and planet formation process is traced by deuterium fractionation. We report here the first detection of doubly deuterated methanol towards pre-stellar cores. We study the deuterium fractionation…

星系天体物理 · 物理学 2023-01-11 Yuxin Lin , Silvia Spezzano , Paola Caselli

In 2013, we have published the first rotational analysis and detection of mono-deuterated dimethyl ether in the solar-type protostar IRAS 16293-2422 with the IRAM 30m telescope. Dimethyl ether is one of the most abundant complex organic…

星系天体物理 · 物理学 2021-07-28 C. Richard , J. K. Jørgensen , L. Margulès , R. A. Motiyenko , J. -C. Guillemin , P. Groner

The millimeter-wave rotational transition line ($J_K = 1_0 - 0_0$) of deuterated methane CH$_3$D has tentatively been detected toward the low-mass Class 0 protostar IRAS 04368+2557 in L1527 with the Heinrich Hertz Submillimeter Telescope.…

太阳与恒星天体物理 · 物理学 2015-06-11 Nami Sakai , Yancy L. Shirley , Takeshi Sakai , Tomoya Hirota , Yoshimasa Watanabe , Satoshi Yamamoto

Recent observations indicate that organic molecules are prevalent towards starless and prestellar cores. Deuteration of these molecules has not been well-studied during the starless phase. Published observations of singly-deuterated…

星系天体物理 · 物理学 2020-12-02 Hannah E. Ambrose , Yancy L. Shirley , Samantha Scibelli

Deuterated molecules are a useful diagnostic tool to probe the evolution and the kinematics in the earliest stages of star formation. Due to the low temperatures and high densities in the centre of pre-stellar cores, the deuterium fraction…

星系天体物理 · 物理学 2026-01-23 K. Giers , S. Spezzano , Y. Lin , P. Caselli , O. Sipilä

Spectra of doubly deuterated propylene oxide, CH$_3$CHCD$_2$O, were recorded in the millimeter-wave spectral region up to 330 GHz utilizing a 2f frequency modulated Terahertz spectrometer. Rotational and centrifugal distortion constants and…

化学物理 · 物理学 2021-08-18 Pascal Stahl , Denis Kargin , Rudolf Pietschnig , Thomas F. Giesen , Guido W. Fuchs

The deuteration of molecules forming in the ices such as methanol (CH$_3$OH) is sensitive to the physical conditions during their formation in dense cold clouds and can be probed through observations of deuterated methanol in hot cores.…

Solar-type prestellar cores and protostars display large amounts of deuterated organic molecules. Recent findings on CHD$_2$OH and CD$_3$OH toward IRAS 16293-2422 suggest that even fully deuterated methanol, CD$_3$OD, may be detectable as…

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