Kazushi Sakamoto: The Kinematics and Dynamics of Molecular Gas in Galactic Centers

Driving gas into Galactic centers
  • opposing torques at corotation point drives gas inward
  • observational evidence from nearby galaxies
  • barred galaxies have greater concentration (Sheth et al 2005)
  • observations of CO gas kinematics in M83, NGC 1097 + FCRAO Quarry obs
  • ALMA concentration to M83 core... + high velocity gas near core + southern nucleus has spatially distinct outflow lobes

Questions

  • Q Fred Lo: Can you distinguish between streamline convergence and cloud collisions? Can you determine what happens when clouds collide?
  • A: Yes, with ALMA.
  • Q Farhad: Physical conditions in NGC 253. Temperature distribution? All warm?
  • A: Our obs don't measure temperature. CO gives 50K on 10's of pc scales, so at least that temperature.
  • Q: Big bubbles in NGC 253. Are there clusters near them?
  • A: Didn't find any in original data.

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