Mapping vinyl cyanide and other nitriles in Titan’s atmosphere using ALMA
Vinyl cyanide (C2H3CN) is theorized to form in Titan's atmosphere via high-altitude photochemistry and is of interest regarding the astrobiology of cold planetary surfaces due to its predicted ability to form cell membrane-like structures (azotosomes) in liquid methane. In this work, we follow...
| Huvudupphovsmän: | , , , , , , , , , , , |
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| Materialtyp: | Journal article |
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American Astronomical Society
2017
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