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Bar-driven Evolution and Instability of Self-gravitating Disks

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Presentation on theme: "Bar-driven Evolution and Instability of Self-gravitating Disks"— Presentation transcript:

1 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

2 Three Observational Facts
Starburst rings Dense circumnuclear molecular disks Gas depression central regions

3 Starburst Rings NGC4313 NGC1512 NGC6782

4 Circumnuclear Disk in ngc1068

5 Center of M51

6 The 3-kpc Arm

7 Gas Distribution in the Milky Way

8 CO and HCN in the Milky Way

9 Distribution of Gas in Galactic Disks

10 Diamond-shaped Ring in NGC6782

11 NGC 1068 Type : Sb / AGN Distance : 14.4 Mpc ( H0 = 75 km s-1 Mpc-1 )
1 arcsec = 74 pc 9.5 arcmin

12 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.

13 Governing Equations

14 Schematic Picture of a Bar
In Numerical Simulations

15 Nearly Flat Rotation Curve
OILR OLR

16 Cases of Double Resonances: OLR-OILR

17 Double Ring Feature

18 Elmegreen Rotation Curve

19 Cases for a Single OLR

20 Evolution of Self-gravitating Disks

21 Double Rings and Central Spirals

22 Double Rings and Central Spirals

23 Q-value for Self-gravitating Disk

24 Onset of Instability

25 Disk Instability

26 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).

27 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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