Potential spectral lines of ethanimine (CH<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si4.svg" display="inline" id="d1e14721"><mml:msub><mml:mrow /><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msub></mml:math>CHNH) - an important possible precursor of amino acids-Reference-Cited by-同舟云学术

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Potential spectral lines of ethanimine (CH3CHNH) - an important possible precursor of amino acids

Published:2023-01 Issue: Volume:98 Page:101928
ISSN:1384-1076
Container-title:New Astronomy
language:en
Short-container-title:New Astronomy

Author:

Sharma Mohit K.,Melosso Mattia^ORCID,Chandra Suresh

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics,Instrumentation

Reference24 articles.

1. Microwave–spectrum of (Z)-ethanimine;Brown;Aust. J. Chem.,1980

2. Collisional rates for asymmetrical top molecules;Chandra;Astron. Astrophys. Suppl.,2000

3. Suggestion for the search of H2CC in cool cosmic objects;Chandra;New Astron.,2011

4. Anomalous absorption in thioformaldehyde;Chandra;New Astron.,2010

5. Anomalous absorption in H2CO molecule;Chandra;Bull. Astron. Soc. India,2006

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. On the Formation of Vinylamine (C₂H₃NH₂) in Interstellar Ice Analogs;The Astrophysical Journal;2023-07-24

2. Advances in the Production of Theanine by Plants and Microorganisms;Fermentation;2023-06-05

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