Making Intermediate mass black holes around Supermassive black holes: like making Jupiters around stars

dc.contributor.author	McKernan, Barry	en
dc.contributor.author	Ford, S.	en
dc.contributor.author	Kocsis, B.	en
dc.contributor.author	Lyra, Wladimir	en
dc.date.accessioned	2017-10-11T21:49:19Z
dc.date.available	2017-10-11T21:49:19Z
dc.date.issued	2014	en
dc.identifier.citation	Bulletin of the American Astronomical Society 46(2). (2014)	en
dc.identifier.other	http://adsabs.harvard.edu/abs/2014AAS...22322302M	en
dc.identifier.uri	http://hdl.handle.net/10211.3/197069	en
dc.description.abstract	Stellar mass black hole seeds can rapidly grow into intermediate mass black holes (IMBH) in accretion disks around supermassive black holes. Initial seed growth is dominated by collisions with stars and later seed growth is dominated by gas accretion. IMBH grow much faster in this model than in globular cluster. There are strong theoretical and observational analogies with the growth of Jupiters in disks around stars. I discuss the growth and observational signatures of IMBH in AGN disks.	en
dc.language.iso	en	en
dc.publisher	American Astronomical Society Meeting Abstracts# 223	en
dc.title	Making Intermediate mass black holes around Supermassive black holes: like making Jupiters around stars	en
dc.type	Conference paper or proceedings	en

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