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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2167
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dc.contributor.authorLokanadham, B-
dc.contributor.authorBabu, G. S. D-
dc.contributor.authorKiron, Y. R-
dc.date.accessioned2008-03-28T09:30:30Z-
dc.date.available2008-03-28T09:30:30Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 413 - 418en
dc.identifier.urihttp://hdl.handle.net/2248/2167-
dc.description.abstractCCD observations of NGC1068 have been obtained in BVRI filters with 2.34 meter Vainu Bappu Telescope of Kavalur in India. The contours of the indices B-V, B-I and V-I of the galaxy indicate the presence of the star-forming region in the circumnuclear ring. The excitation mechanism of the star forming complexes is explained in the light of multi-wavelength observations of the galaxy.en
dc.format.extent454266 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..413Len
dc.subjectGalaxiesen
dc.subjectSeyfertsen
dc.subjectNGC1068en
dc.subjectStructureen
dc.titleCCD imaging of Seyfert galaxy NGC 1068en
dc.typeArticleen
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