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Updated: Apr 25, 2026

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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巨大的恒星. 巨大的恒星. 第一代非常大质量的恒星的化学特征

W Aoki1, N Tominaga2, T C Beers3

  • 1National Astronomical Observatory of Japan (NAOJ), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan. Department of Astronomical Science, School of Physical Sciences, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan. aoki.wako@nao.ac.jp.

Science (New York, N.Y.)
|August 23, 2014
PubMed
概括

研究人员分析了一颗缺乏金属的恒星,SDSS J001820.5-093939.2,发现了独特的元素丰度. 这些图案表明,它是由一个非常大质量的恒星的超新星形成的,可能超过100个太阳质量.

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