Optical microvariability in radio quiet quasars

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DC Field	Value	Language
dc.contributor.author	Wiita, P. J	-
dc.contributor.author	Gopal-Krishna	-
dc.contributor.author	Sagar, R	-
dc.date.accessioned	2008-12-15T16:37:40Z	-
dc.date.available	2008-12-15T16:37:40Z	-
dc.date.issued	1994	-
dc.identifier.citation	IAU Symposium Vol. 159, pp. 414	en
dc.identifier.uri	http://hdl.handle.net/2248/4064	-
dc.description.abstract	We have observed 11 radio quiet QSOs (RQQSOs) to see if they exhibit intranight variability in the optical. The detection of such microvariability would support models in which flutuations on accretion disks are dominant, while if it is never present, modles based on relativistic jets would be favored. Although several of these RQQSOs show hints of microvrariability, we cannot claim to have discovered this phenomenon in this class of objects. Several of the comparison stars have clearly shown rapid variability.	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994IAUS..159..414W	en
dc.title	Optical microvariability in radio quiet quasars	en
dc.type	Article	en
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