Physics and observations of tidal disruption events

dc.contributor.author	Mangalam, A
dc.contributor.author	Mageshwaran, T
dc.date.accessioned	2020-11-11T01:15:26Z
dc.date.available	2020-11-11T01:15:26Z
dc.date.issued	2018-04
dc.identifier.citation	Bulletin de la Société Royale des Sciences de Liège, Vol. 87, Actes de colloques, 2018, p. 307– 315	en_US
dc.identifier.issn	0037-9565
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6837
dc.description	Open Access ©Societe Royale des Sciences de Liege; https://popups.uliege.be/0037-9565/index.php?id=7747	en_US
dc.description.abstract	We describe a model of tidal disruption events (TDEs) with input physical parameters that include the black hole (BH) mass M•, the specific orbital energy E, the angular momentum J, the star mass M? and radius R?. We calculate the rise time of the TDEs, the peak bolometric luminosity in terms of these physical parameters and a typical light curve of TDEs for various All Sky Survey (ASS) and Deep Sky Survey (DSS) missions. We then derive the expected detection rates and discuss the follow up of TDEs through observations in various spectral bands from X-rays to radio wavelengths.	en_US
dc.language.iso	en	en_US
dc.publisher	Societe Royale des Sciences de Liege	en_US
dc.subject	Astronomy	en_US
dc.subject	Astrophysics	en_US
dc.subject	Black hole	en_US
dc.subject	Disruption	en_US
dc.subject	Modelling	en_US
dc.title	Physics and observations of tidal disruption events	en_US
dc.type	Article	en_US