A search for rapid coptical variability in low-mass seyfert galaxies: NGC 4395

dc.contributor.author	Semkov, E.
dc.contributor.author	Bachev, R.
dc.contributor.author	Strigachev, A.
dc.contributor.author	Peneva, S.
dc.contributor.author	Gupta, A. C.
dc.date.accessioned	2015-04-27T11:22:06Z
dc.date.available	2015-04-27T11:22:06Z
dc.date.issued	2011
dc.identifier.uri	http://hdl.handle.net/123456789/989
dc.description.abstract	We present first results of a program to monitor active galactic nuclei with intermediate mass black holes. The monitoring aims to search for rapid (intranight) optical variations in these objects, most of which are known to show significant X-ray variability on minutes-to-hours timescales. Finding optical counterpart of the higher energy variations might be of important for the modelling of the innermost regions of these objects. This paper presents the results for NGC 4395 the lowest mass AGN known so far.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	baj17-46
dc.subject	Active galactic nuclei, quasars, variablity, individual - NGC 4395	en_US
dc.title	A search for rapid coptical variability in low-mass seyfert galaxies: NGC 4395	en_US
dc.type	Article	en_US