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Bar-driven Evolution and Instability of Self-gravitating Disks
Chi Yuan Institute of Astronomy and Astrophysics Academia Sinica, Taipei, Taiwan, ROC David C.C. Yen, Yi-Hsin Liu, Chao-Chin Yang
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Three Observational Facts
Starburst rings Dense circumnuclear molecular disks Gas depression central regions
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Starburst Rings NGC4313 NGC1512 NGC6782
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Circumnuclear Disk in ngc1068
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Center of M51
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The 3-kpc Arm
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Gas Distribution in the Milky Way
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CO and HCN in the Milky Way
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Distribution of Gas in Galactic Disks
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Diamond-shaped Ring in NGC6782
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NGC 1068 Type : Sb / AGN Distance : 14.4 Mpc ( H0 = 75 km s-1 Mpc-1 )
1 arcsec = 74 pc 9.5 arcmin
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The Antares Code 大火程序 A high-performance CFD-MHD code for astrophysics
It is a second-order Godunov code (or codes) equipped with exact Riemann solver and the balance law correction. (2-D) It is also featured with the fft Poisson solver, to include the self-gravitation of the disk, and with characteristics decomposition on the boundary, to guarantee the true radiation (non-reflecting) boundary conditions.
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Governing Equations
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Schematic Picture of a Bar
In Numerical Simulations
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Nearly Flat Rotation Curve
OILR OLR
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Cases of Double Resonances: OLR-OILR
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Double Ring Feature
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Elmegreen Rotation Curve
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Cases for a Single OLR
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Evolution of Self-gravitating Disks
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Double Rings and Central Spirals
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Double Rings and Central Spirals
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Q-value for Self-gravitating Disk
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Onset of Instability
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Disk Instability
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A fast nuclear bar like possibly NGC4313 (OLR).
Conclusions Starburst rings are the results of a gaseous disk responding to a rotating bar potential. But, there are many possibilities. A fast nuclear bar like NGC1068 or the Milky Way (OLR and OILR) A fast nuclear bar like possibly NGC4313 (OLR).
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Conclusions cont. A double ring due slow bar like NGC6278 (OLR-OILR).
A fast bar in the center solves the starburst ring, dense circumnuclear molecular disk, and depletion of gas in between all together. Self-gravitation plays an important role. It leads to instability, chaos, and star formation Toomre’s criterion Q=1 works extremely well.
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