Is the binding energy of galaxies related to their core black hole mass?

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	Arun, K	-
dc.date.accessioned	2021-07-23T05:33:13Z	-
dc.date.available	2021-07-23T05:33:13Z	-
dc.date.issued	2021-10	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 42, No. 2, 12	en_US
dc.identifier.issn	0973-7758	-
dc.identifier.uri	http://hdl.handle.net/2248/7811	-
dc.description	Restricted Access	en_US
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	Most of the large galaxies host a supermassive black hole, but their origin is still not well understood. In this paper, we look at a possible connection between the gravitational binding energies of large galaxies, etc., and the masses of their central black holes. Using this relation (between the gravitational binding energy of the host structure and the black hole energy), we argue why globular clusters are unlikely to harbour large black holes and why dwarf galaxies, if they have to host black holes, should have observed mass-to-light ratios of ~100.	en_US
dc.language.iso	en	en_US
dc.publisher	Indian Academy of Sciences	en_US
dc.relation.uri	https://doi.org/10.1007/s12036-021-09732-4	-
dc.rights	© Indian Academy of Sciences	-
dc.subject	Binding energy	en_US
dc.subject	Black holes	en_US
dc.subject	Dwarf galaxies	en_US
dc.title	Is the binding energy of galaxies related to their core black hole mass?	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

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