Reinhardt Genzel 20/10/2009

Max Planck Institut für Extraterrestrische Physik, Alemania University of California at Berkeley, EE.UU.
Madrid, 20 de octubre de 2009 Evidence has been accumulating for several decades that many galaxies harbor central mass concentrations that may be in the form of black holes with masses between a few million to a few billion time the mass of the Sun. I will discuss measurements over the last two decades, employing adaptive optics imaging and spectroscopy on large ground-based telescopes that prove the existence of such a massive black hole in the Center of our Milky Way, beyond any reasonable doubt. These data also provide key insights into its properties and environment. Future interferometric studies of the Galactic Center black hole promise to be able to test gravity in its strong field limit. I will also briefly discuss the cosmological evolution of massive black holes.

Vídeos
Ciencias de la vida y de la materia Herederos de Galileo

Michel Mayor 28/10/2009

Acto de Clausura

Brian Schmidt 19/10/2009

Roger Chevalier 21/10/2009

Peter Schneider 21/10/2009

Reinhardt Genzel 20/10/2009

Luis Felipe Rodríguez 20/10/2009

Esteban Domingo 20/10/2009

Jose María Torrelles 20/10/2009

Eduard Salvador 20/10/2009

Xavier Barcons

Rafael Rebollo López 19/10/2009

Michel Mayor 19/10/2009

Mike Brown 19/10/2009

Roberto Gilmozzi 19/10/2009

William Shea 19/10/2009

Inauguración Herederos de Galileo 19/10/2009