Reverberation mapping of the Seyfert 1.5 galaxy H 0507+164

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5905

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DC Field	Value	Language
dc.contributor.author	Jeyakumar, S	-
dc.contributor.author	Stalin, C. S	-
dc.contributor.author	Coziol, R	-
dc.date.accessioned	2012-09-17T10:57:42Z	-
dc.date.available	2012-09-17T10:57:42Z	-
dc.date.issued	2011-10	-
dc.identifier.citation	XIII Latin American Regional IAU Meeting,Morelia, Michoacán, México, November 8 - 12, 2010, edited by W. J. Henney & S. Torres-Peimbert, Rev. Mex. AA (Serie de Conferencias), Vol. 40, pp. 123	en
dc.identifier.isbn	978-607-02-2653-3	-
dc.identifier.uri	http://hdl.handle.net/2248/5905	-
dc.description	Open Access	en
dc.description.abstract	Light curves of the continuum at 5100 °A and Hβ line are obtained from spectroscopic monitoring observations of the Seyfert 1.5 galaxy H 0507+164. The mass of the black hole is calculated based on cross-correlation analysis of these light curves.	en
dc.language.iso	en	en
dc.publisher	Instituto de Astronomia, UNAM	en
dc.relation.uri	http://www.astroscu.unam.mx/~rmaa/rmaa.html	en
dc.rights	© Instituto de Astronomia, UNAM - XIII Latin American Regional IAU Meeting	en
dc.subject	Galaxy	en
dc.subject	Seyfert 1.5 Galaxy H 0507+164	en
dc.subject	Active Galactic Nuclei (AGNs)	-
dc.title	Reverberation mapping of the Seyfert 1.5 galaxy H 0507+164	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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