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DTSTART:20151025T010000
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DTSTART;TZID=Europe/Rome:20160223T114500
DTEND;TZID=Europe/Rome:20160223T124500
DTSTAMP:20260413T042023
CREATED:20160216T153808Z
LAST-MODIFIED:20160216T153808Z
UID:451-1456227900-1456231500@www.oa-roma.inaf.it
SUMMARY:Linking massive black hole spin evolution to galactic dynamics
DESCRIPTION:The evolution of the spin of massive black holes (MBHs) is driven by accretion of gas and/or by black hole binary coalescences. I will discuss the physical processes involved in the MBH spin evolution\, and present the results of a semi-analytical model that manages to reproduce the distribution of spins obtained from X-ray spectroscopy.
URL:https://www.oa-roma.inaf.it/event/linking-massive-black-hole-spin-evolution-to-galactic-dynamics/
LOCATION:Aula Gratton
CATEGORIES:Seminari
ORGANIZER;CN="OAR":MAILTO:info@oa-roma.inaf.it
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20160223T114500
DTEND;TZID=Europe/Rome:20160223T124500
DTSTAMP:20260413T042023
CREATED:20160216T153808Z
LAST-MODIFIED:20160216T153808Z
UID:4653-1456227900-1456231500@www.oa-roma.inaf.it
SUMMARY:Linking massive black hole spin evolution to galactic dynamics
DESCRIPTION:The evolution of the spin of massive black holes (MBHs) is driven by accretion of gas and/or by black hole binary coalescences. I will discuss the physical processes involved in the MBH spin evolution\, and present the results of a semi-analytical model that manages to reproduce the distribution of spins obtained from X-ray spectroscopy.
URL:https://www.oa-roma.inaf.it/event/linking-massive-black-hole-spin-evolution-to-galactic-dynamics-2/
LOCATION:Aula Gratton
CATEGORIES:Seminari
ORGANIZER;CN="OAR":MAILTO:info@oa-roma.inaf.it
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