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SMP on SMBH Are these two empirical laws similar? The same? Isothermal spheres Isothermal distribution functions Isothermal singular sphere Isothermal non-singular sphere Conclusions for the magnitude of dynamical friction in dark halos: the reason for efficient mergers Rotation and flattening of elliptical

SMP on SMBH Are these two empirical laws similar? The same? Isothermal spheres

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ASTC22. Lectures L20 SMP: Supermassive Black Holes Faber-Jackson vs. Tully-Fisher. SMP on SMBH Are these two empirical laws similar? The same? Isothermal spheres Isothermal distribution functions Isothermal singular sphere Isothermal non-singular sphere - PowerPoint PPT Presentation

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Page 1: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

SMP on SMBH

Are these two empirical laws similar? The same? Isothermal spheres Isothermal distribution functions Isothermal singular sphere Isothermal non-singular sphere Conclusions for the magnitude of dynamical friction in dark halos: the reason for efficient mergers Rotation and flattening of elliptical galaxies: only a weak

connection

Page 2: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 3: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

Even the fantastic resolution ofthe VLBI radio interferometrycannot resolve the central engine.The dot in the lower left corner is of order 6 Schwarzschild radii,

i.e. several times the size of the black hole event horizon, from within which light or information cannot escape.

Page 4: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 5: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 6: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

Empirical correlation exists between the supermassive black hole mass and the luminosity (and thus mass) of the bulge of the host galaxy, M87 isshown in a red circle

Page 7: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

SMP on SMBHs

Page 8: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

Tully-Fisher relationship, a correlation between the luminosityand rotation for diskgalaxies

Log

Vc

-2.5 log L

Page 9: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

Faber-Jackson relationship:Luminosity ~ sigma^4 applies to ellipticals

Tully-Fisher relationshipLuminosity ~ (Vc)^3.85applies to disk galaxies

but the two are almost identical:both the disks and the ellipticalsare immersed in the same typeof dark halos which determinesthe maximum Vc via potentialwell depth.

Page 10: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 11: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 12: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

(sorry, that’smy teenage daughter)

Page 13: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

Good for modelingflat-Vc galaxiesin dark halos

Page 14: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 15: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres
Page 16: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

...so this is one major reason why mergers of galactic systems areso rapid (a few to a few dozen periods)

Page 17: SMP on SMBH Are these two empirical laws similar? The same?   Isothermal spheres

One more empirical correlation: between rotation and flattening of ellipticals, which can be understood based on stellar dynamics

Fastest rotation according to theory

But remember: theory gives the upper envelope only. Most ellipticals are NOT supported or flattened by rotation. They simply are not relaxed; flatteningcomes from initial conditions, including geometry of encounter.