The Galactic Center Molecular Tornado Driven by Magnetic Squeezing Mechanism
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2007-02-25
著者
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SOFUE Yoshiaki
Institute of Astronomy, The University of Tokyo
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Sofue Yoshiaki
Institute Of Astronomy The University Of Tokyo
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Sofue Yoshiaki
Institute Of Astronomy Faculty Of Science The University Of Tokyo
関連論文
- Three-Dimensional Distribution of the ISM in the Milky Way Galaxy : II. The Molecular Gas Disk
- A Chain of Dark Clouds in Projection Against the Galactic Center
- Nobeyama Millimeter Array Observations of GRB 030329 : a Decay of Afterglow with Bumps and Molecular Gas in the Host Galaxy
- ASTE ^CO (J = 3-2) Survey of Elliptical Galaxies
- Hubble Constant at Intermediate Redshift Using the CO-Line Tully-Fisher Relation
- CO Observations of Luminous IR Galaxies at Intermediate Redshift
- Distance Measurement of Galaxies to a Redshift of-0.1 Using the CO-Line Tully-Fisher Relation
- The Virgo High-Resolution CO Survey : III. NGC 4254
- Three-Dimensional Distribution of the ISM in the Milky Way Galaxy : I. The HI Disk
- ASTE Observations of Nearby Galaxies : A Tight Correlation between CO (J = 3-2) Emission and Hα
- Virgo High-Resolution CO Survey : V. Circumnuclear Elliptical Ring in NGC 4569
- The Schmidt Law at High Molecular Densities
- The Virgo High-Resolution CO Survey : II. Rotation Curves and Dynamical Mass Distributions
- The Virgo High-Resolution CO Survey : I. CO Atlas
- Threshold between Spontaneous and Cloud-Collisional Star Formation
- Offsets between Hα and CO Arms of a Spiral Galaxy, NGC 4254 : A New Method for Determining the Pattern Speed of Spiral Galaxies
- Virgo High-Resolution CO Survey : IV. Spiral-Driven Gas Dynamics in the Non-Barred Seyfert Galaxy NGC 4501
- Effects of Starbursts on the Structure of Young Galaxies
- Why Can We Detect the High-Redshift Quasar BR 1202-0725 in CO?
- The Virgo High-Resolution CO Survey : VI. Gas Dynamics and Star Formation along the Bar in NGC 4303
- The Galactic Center Molecular Tornado Driven by Magnetic Squeezing Mechanism
- Magnetic-Reconnection and Current-Sheet Model for the Radio Arc and Threads in the Galactic Center
- Galactic Center Shells and a Recurrent Starburst Model
- H I Jet G40-15 from a Rotating Cloud in the 4-kpc Molecular Ring : Magnetized Outflow and Formation of a Dense Star Cluster
- Distance Measurement of Spiral Arms in the Galactic-Center Direction Using Radial-Velocity Gradients
- Central Kinematics and Rotation Curve of the Sb Galaxy NGC 4527 in CO, Hα, and [N II] Lines
- OPtical and CO Radio Observations of Poor Cluster Zwicky 1615.8+3505
- Nuclear-to-Disk Rotation Curves of Galaxies in the Hα and[NII]Emission Lines
- Dark Bulge, Exponential Disk, and Massive Halo in the Large Magellanic Cloud
- CO-to-H_2 Conversion Factor in Galaxies
- Distribution and Dynamics of Molecular Gas in the Galaxy M51. II. Formation of Giant Molecular Associations and Massive Stars
- Ram-Pressure Effects on Dense Molecular Arms in the Central Regions of Spiral Galaxies by Intracluster Medium
- Mass of the Galaxy Inferred from Outer Rotation Curve
- Is M82 a Disk-Truncated Bulge by a Close Encouter with M81?
- Spiral Molecular Front in Galaxies: Quick Transition from Atomic to Molecular Hydrogen in Spiral Arms
- Rotation Curve of the Galaxy
- On the Keplerian Rotation Curves of Galaxies
- 150 GHz NOBA Observations of the Galactic Center Arc
- Kinematical Properties of Giant Molecular Clouds and Star Forming Efficiency
- Galactic-Center Molecular Arms, Ring, and Expanding Shell. I. Kinematical Structures in Longitude-Velocity Diagrams
- Nuclear-to-Outer Rotation Curves of Galaxies in the CO and H_I Lines