Skip to content

Title: Supermassive black holes in the Universe

Speaker: Jian-Min Wang

Outlines

  • Formation of SMBHs
  • Masses and spins
  • SMBH binaries and nanohertz GWs
  • Satellite BHs and observational consequences
  • Opportunities in the era of JWST and VLTI

First quasar: 3C 273

Fig1
Fig2

So broad Hβ emission

Formation of SMBHs

Fig3
Fig4

Does the mass of BH grow first or that of the host galaxy?

The masses of BHs are mainly from accretion. SMBHs favor super-Eddington accretion.

Fig5

Masses an spins

Fig6

“It is hard to say that the spin depends on the mass.”

SMBH binaries and nanohertz GWs

Fig7

Pile-up mass function

Fig8

Released under the MIT License.