Shock Waves and Line-Profile Variation in roAp Stars
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2008-02-25
著者
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SHIBAHASHI Hiromoto
Department of Astronomy, School of Science, The University of Tokyo
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Kurtz Donald
Centre For Astrophysics University Of Central Lancashire
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Kambe Eiji
Okayama Astrophysical Observatory National Astronomical Observatory
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GOUGH Douglas
Institute of Astronomy
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Shibahashi Hiromoto
Department Of Astronomy School Of Science The University Of Tokyo
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Shibahashi Hiromoto
Department Of Astronomy The University Of Tokyo
関連論文
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- Planetary Companions to Evolved Intermediate-Mass Stars : 14 Andromedae, 81 Ceti, 6 Lyncis, and HD 167042
- Planetary Companions around Three Intermediate-Mass G and K Giants : 18 Delphini, ξ Aquilae, and HD 81688
- Detection of Small-Amplitude Oscillations in the G-Giant HD 76294 (ζ Hydrae)
- Development of Iodine Cells for Subaru HDS and Okayama HIDES. III : An Improvement on the Radial-Velocity Measurement Technique
- Dramatic Spectral and Photometric Changes of Pleione (28 Tau) between 2005 November and 2007 April
- Initial Helioseismic Observations by Hinode/SOT
- Observations of Sunspot Oscillations in G Band and Ca II H Line with Solar Optical Telescope on Hinode
- A Massive Substellar Companion to the Massive Giant HD 119445
- Oxygen and Neon Abundances of B-Type Stars in Comparison with the Sun
- Shock Waves and Line-Profile Variation in roAp Stars
- An Abundance Analysis of the Primary Star of the Peculiar Eclipsing Binary ε Aurigae out of the Eclipsing Phase
- 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
- Drastic Spectroscopic Variability of the Be/X-Ray Binary Ariel 0535+262/V725 Tau during and after the 2009 Giant Outburst
- 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
- A Planetary Companion to the Intermediate-Mass Giant HD 100655
- Vibrational Instability of Population III Low-Mass Stars due to the ε-Mechanism
- Substellar Companions to Seven Evolved Intermediate-Mass Stars