A super compact object sitting in the center of an elliptical galaxy may start a strong gravitational activity due to aspherical mass accretion in the form of dynamically braked globular clusters as well as in the form of stellar debris of tidally destroyed clusters. The resulting AGN luminosity and life time depend mainly on the black hole size and initial characteristics of the globular cluster family.
Gravitational Waves Generated by Globular Cluster Systems Collapse / CAPUZZO DOLCETTA, Roberto Angelo; Miocchi, Paolo. - STAMPA. - (1998), pp. 481-481. ( IAU SYMPOSIUM NO. 184 "THE CENTRAL REGIONS OF THE GALAXY AND GALAXIES Kyoto (Japan) 18-22 August 1997).
Gravitational Waves Generated by Globular Cluster Systems Collapse
CAPUZZO DOLCETTA, Roberto Angelo;MIOCCHI, PAOLO
1998
Abstract
A super compact object sitting in the center of an elliptical galaxy may start a strong gravitational activity due to aspherical mass accretion in the form of dynamically braked globular clusters as well as in the form of stellar debris of tidally destroyed clusters. The resulting AGN luminosity and life time depend mainly on the black hole size and initial characteristics of the globular cluster family.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
