Bisymmetric Spiral Configuration of Magnetic Fields in Spiral Galaxies-2-A Quasi-Global Theory
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関連論文
- 球状星団の形成と銀河の衝突史--マゼラン雲の歴史をたどる
- 大小マゼラン雲の衝突史とマゼラン電流(天文学の境界領域を探る,研究会報告)
- 銀河と宇宙の磁場
- Bisymmetric Spiral Configuration of Magnetic Fields in Spiral Galaxies-2-A Quasi-Global Theory
- Bisymmetric Spiral Configuration of Magnetic Fields in Spiral Galaxies-1-Local Theory
- Asymmetric Distribution of Gas in the Large Magellanic Cloud and Dynamical Condition for Globular Cluster Formation
- Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
- The Vertical Large-Scale Magnetic Fields in Spiral Galaxies
- Instability of Interaction Network for Interstellar Gas and Interstellar Diffusive Energy in the Shear Field
- An Upper Limit on the Mean Mass of Black Holes in the Galactic Halo
- Velocity Dispersion of Stars and Giant Molecular Clouds
- Numerical Simulation for Stellar Velocity Dispersion and Hardness of Encounters between Stars and Perturbers
- Dynamical Evolution of Galactic Disk Stars Due to Giant Molecular Clouds and Spiral Density Waves
- Dynamical Evolution of Galactic Disk Stars Due to Giant Molecular Clouds and Spiral Density Waves-2-
- Dynamics of Rotating Gaseous Ellipsoid in External Force Fields