Detectable abundance of cyanoacetylene (HC3N) predicted on reduced nitrogen-rich super-earth atmospheres

被引:0
|
作者
Rimmer, Paul B. [1 ,2 ,3 ]
Majumdar, Liton [4 ]
Priyadarshi, Akshay [5 ]
Wright, Sam [6 ]
Yurchenko, S.N. [6 ]
机构
[1] Department of Earth Sciences, University of Cambridge, Downing St, Cambridge,CB2 3EQ, United Kingdom
[2] Cavendish Laboratory, University of Cambridge, JJ Thomson Ave, Cambridge,CB3 0HE, United Kingdom
[3] MRC Laboratory of Molecular Biology, Francis Crick Ave, Cambridge,CB2 0QH, United Kingdom
[4] School of Earth and Planetary Sciences, National Institute of Science Education and Research, HBNI, Jatni, Odisha,752050, India
[5] School of Physical Sciences, National Institute of Science Education and Research, HBNI, Jatni, Odisha,752050, India
[6] Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom
来源
arXiv | 2021年
关键词
657.2 Extraterrestrial Physics and Stellar Phenomena - 701 Electricity and Magnetism - 741.3 Optical Devices and Systems - 804 Chemical Products Generally;
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学科分类号
摘要
Extrasolar planets
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