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Updated: Jun 24, 2025

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
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Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

Published on: February 19, 2018

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質量 が 極めて 低い 恒星 の 円盤 に ある 炭化 素 の 豊富 な 量

A M Arabhavi1, I Kamp1, Th Henning2

  • 1Kapteyn Astronomical Institute, University of Groningen, Groningen 9700 AV, Netherlands.

Science (New York, N.Y.)
|June 6, 2024
PubMed
まとめ

質量が非常に低い星は 惑星を頻繁に宿している. ジェームズ・ウェブ宇宙望遠鏡の観測により,若い恒星の周りの炭素が豊富な円盤が明らかになり,そこに形成された地上の惑星は,豊富な炭化水素によるユニークな組成を持つ可能性があることを示唆しています.

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