"The Biggest Black
Holes"
Dr.
Amri Wandel
Racah
Institute of Physics, The Hebrew University
In recent years Massive Black Holes (MBHs) with masses of 106-109
times
the mass of the sun, have been detected in the centers of many galaxies,
including our own, using stellar and gas motions. As more MBHs were measured,
an amazing result emerged: the masses of the MBHs are a fraction
(0.002-0.005) of the host galaxy (Richstone 1998 et al.,Nature 395, A14).
MBHs have been measured also in the nuclei of active galaxies and quasars,
using the new reverberation technique. These MBHs seem to show a similar
mass relation, but by a factor of ~10 lower than in less active and ordinary
galaxies.
Understanding these observations can answer some facinating questions:
Does every galaxy have a MBH at its center? How do MBHs evolve? Did nonactive
MBHs, such as in our Galaxy, have an active past as quasars or active nuclei?
Host:
Dr. Ron Lifshitz, x5145
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