Origin of High-Speed Non-Thermal Flow Due to the Collisions of Molecular Cloud Clumps
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概要
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関連論文
- Implication of Dark Matter in Dwarf Spheroidal Galaxies
- A Nonlinear-Open-System Model for Star Formation in Spiral Galaxies
- Conversion Law of Infrared Luminosity to Star-Formation Rate for Galaxies
- Zeeman Spectrum from a Magnetically Triggered Jet
- Evolution of Hydromagnetic Disturbances in Low Ionized Cosmic Plasmas
- Structural Model of Molecular Cloud Complexes: Mass, Size, and External Pressure
- Interstellar-Cloud Formation in the Extended Envelopes of Blue Compact Dwarf Galaxies
- Origin of High-Speed Non-Thermal Flow Due to the Collisions of Molecular Cloud Clumps
- Stability Condition of the Kelvin-Helmholtz Instability for the Two-Component Protogalaxy
- Damping Efficiency of the Void Mode in a Two-Phase Gas Mixture with a Phase Transition
- H_2 Formation in Low-Metallicity Galaxies
- Interpretation of the Expansion Law of Planetary Nebulae
- Amplification of Magnetic Fields in an Accretion Disk with a Starburst Torus
- Intergalactic dust and its photoelectric heating
- Wave Dispersion in a Two-Phase Gas Mixture : Comments on Random Motions and Void Modes
- Comments on a Formation Scenario of the Two-Component Protogalaxy by Galactic Magnetic Fields