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  • 标题:Laboratory measurements and astronomical search for cyanomethanimine ⋆
  • 本地全文:下载
  • 作者:M. Melosso ; A. Melli ; C. Puzzarini
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2018
  • 卷号:609
  • DOI:10.1051/0004-6361/201731972
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:Context.C-cyanomethanimine (HNCHCN), existing in the twoZandEisomeric forms, is a key prebiotic molecule, but, so far, only theEisomer has been detected toward the massive star-forming region Sagittarius B2(N) using transitions in the radio wavelength domain.Aims.With the aim of detecting HNCHCN in Sun-like-star forming regions, the laboratory investigation of its rotational spectrum has been extended to the millimeter-/submillimeter-wave (mm-/submm-) spectral window in which several unbiased spectral surveys have been already carried out.Methods.High-resolution laboratory measurements of the rotational spectrum of C-cyanomethanimine were carried out in the 100–420 GHz range using a frequency-modulation absorption spectrometer. We then searched for the C-cyanomethanimine spectral features in the mm-wave range using the high-sensitivity and unbiased spectral surveys obtained with the IRAM 30-m antenna in the ASAI context, the earliest stages of star formation from starless to evolved Class I objects being sampled.Results.For both theZandEisomers, the spectroscopic work has led to an improved and extended knowledge of the spectroscopic parameters, thus providing accurate predictions of the rotational signatures up to~700 GHz. So far, no C-cyanomethanimine emission has been detected toward the ASAI targets, and upper limits of the column density of~1011–1012cm-2could only be derived. Consequently, the C-cyanomethanimine abundances have to be less than a few 10-10for starless and hot-corinos. A less stringent constraint,≤10-9, is obtained for shocks sites.Conclusions.The combination of the upper limits of the abundances of C-cyanomethanimine together with accurate laboratory frequencies up to~700 GHz poses the basis for future higher sensitivity searches around Sun-like-star forming regions. For compact (typically less than 1″) and chemically enriched sources such as hot-corinos, the use of interferometers as NOEMA and ALMA in their extended configurations are clearly needed.
  • 关键词:enISM: moleculesmolecular datamethods: data analysismethods: laboratory: molecular
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