Fully Nonadiabatic Analysis of Vibrational Instability of Population III Stars due to the ε-Mechanism
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概要
- 論文の詳細を見る
- 2012-02-25
著者
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Shibahashi Hiromoto
Department Of Astronomy School Of Science The University Of Tokyo
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Sonoi Takafumi
Department Of Astronomy School Of Science The University Of Tokyo
関連論文
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- Initial Helioseismic Observations by Hinode/SOT
- Observations of Sunspot Oscillations in G Band and Ca II H Line with Solar Optical Telescope on Hinode
- Shock Waves and Line-Profile Variation in roAp Stars
- Solar Models with Helioseismic Constraints and the Solar Neutrino Problem
- A Seismic Solar Model Deduced from the Sound-Speed Distribution and an Estimate of the Neutrino Fluxes
- Hydrogen Abundance in the Tachocline Layer of the Sun
- Numerical Simulations of Line-Profile Variation beyond a Single-Surface Approximation for Oscillations in roAp Stars
- Fully Nonadiabatic Analysis of Vibrational Instability of Population III Stars due to the ε-Mechanism
- Vibrational Instability of Population III Low-Mass Stars due to the ε-Mechanism