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Tentative detection of cyanoformamide NCCONH2in space

  • Juan Li
  • , Donghui Quan
  • , Junzhi Wang
  • , Xia Zhang
  • , Xing Lu
  • , Qian Gou
  • , Feng Gao
  • , Yajun Wu
  • , Edwin Bergin
  • , Shanghuo Li
  • , Zhiqiang Shen
  • , Fujun Du
  • , Meng Li
  • , Siqi Zheng
  • , Xingwu Zheng
  • CAS - Shanghai Astronomical Observatory
  • Chinese Academy of Sciences
  • Research Center for Intelligent Computing Platforms
  • Zhejiang Lab
  • Eastern Kentucky University
  • Guangxi University
  • CAS - National Astronomical Observatories
  • Chongqing University
  • University of Hamburg
  • Max Planck Institute for Radio Astronomy
  • University of Michigan, Ann Arbor
  • Max Planck Institute for Astronomy
  • CAS - Purple Mountain Observatory
  • University of Chinese Academy of Sciences
  • Nanjing University

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

The peptide-like molecule cyanoformamide (NCCONH2) is the cyano (CN) derivative of formamide (NH2CHO). It is known to play a role in the synthesis of nucleic acid precursors under prebiotic conditions. In this paper, we present a tentative detection of NCCONH2 in the interstellar medium with the Atacama Large Millimeter/submillimeter Array (ALMA) archive data. 10 unblended lines of NCCONH2 were seen around 3σ noise levels toward Sagittarius B2(N1E), a position that is slightly offset from the continuum peak. The column density of NCCONH2 was estimated to be 2.4 × 1015 cm-2, and the fractional abundance of NCCONH2 toward Sgr B2(N1E) was 6.9 × 10-10. The abundance ratio between NCCONH2 and NH2CHO is estimated to be ∼0.01. We also searched for other peptide-like molecules toward Sgr B2(N1E). The abundances of NH2CHO, CH3NCO and CH3NHCHO toward Sgr B2(N1E) were about 1/10 of those toward Sgr B2(N1S), while the abundance of CH3CONH2 was only 1/20 of that toward Sgr B2(N1S).

Original languageEnglish
Pages (from-to)54-64
Number of pages11
JournalPublications of the Astronomical Society of Japan
Volume76
Issue number1
DOIs
Publication statusPublished - 1 Feb 2024

Keywords

  • ISM: abundances
  • ISM: clouds
  • ISM: molecules
  • radio lines: ISM
  • SM: individual (Sagittarius B2)

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