Can Galactic Nuclei Activity be Explained by Globular Cluster Mass Accretion?

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dc.creatorCapuzzo-Dolcetta, Roberto
dc.date1996-12-10
dc.date.accessioned2026-07-07T02:22:31Z
dc.date.available2026-07-07T02:22:31Z
dc.descriptionGlobular clusters can decay to the center of their mother galaxy carrying a quantity of mass sufficient to sustain the gravitational activity of a small pre-existing nucleus and to accrete it in a significant way. The AGN luminosity and lifetime depend on the characteristics of the globular cluster system and it is quite insensitive to the nucleus' initial mass.
dc.description4 pages + 1 postscript figure; presented at the Workshop "From Micro- to Mega-Parsec" (Riccione, oct. 7-10, 1996)
dc.identifierhttps://arxiv.org/abs/astro-ph/9612100
dc.identifierhttp://arxiv.org/abs/astro-ph/9612100
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10906
dc.subjectAstrophysics
dc.titleCan Galactic Nuclei Activity be Explained by Globular Cluster Mass Accretion?
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