Contribution to the Helium Content of the Galaxy from Pulsationally Unstable Stars Evolving Inhomogeneously

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概要

• 論文の詳細を見る
• 理論物理学刊行会の論文
• 1971-11-25

著者

• TANAKA Yasuo

  Faculty of Education, Ibaraki University

• Sakashita Shiro

  Department Of Physics Hokkaido University

• Tanaka Yasuo

  Faculty Of Education Ibaraki University

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• Thermal Instability of Hydrogen-Burning Shell in Very Massive Stars
• Flow Patterns of Cluster Winds and X-Ray Emissions from Clusters of Galaxies
• The Appearance of Primeval Galaxies in X- and γ-Ray Regions and Their Contributions to the Background Radiation
• Off-Center Point Explosion in a Spheroid
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• Hamamoto's Remedy for the Band Crossing Anomalies in the Cranking Model
• Stellar Accretion and X-Ray Source. II
• Nonlinear Properties of a Self-Exciting Oscillator
• Propagation of Shock Waves in Inhomogeneous Gases. II : Hydromagnetic Shock
• On the Possibility of Helium Burning in Giant Stars in a Globular Cluster
• The Evolution of Massive Stars. I
• Note on Intermittent Bursts of a Hydrodynamic Model
• Neutrino Pair Emission from Excited Nuclei. II
• Propagation of the General Relativistic Blast Wave
• Contribution to the Helium Content of the Galaxy from Pulsationally Unstable Stars Evolving Inhomogeneously
• Structure-Activity Relationships of Saponins and Cardiac Glycosides. III. β-L-Xylopyranosyl-(1→6)-α- and -β-D-Glucopyranosides
• On the Origin of Planetary Nebulae
• Neutrino Pair Emission from Excited Nuclei
• Stellar Accretion and X-Ray Source

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