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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2118
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dc.contributor.authorKamath, U. S-
dc.date.accessioned2008-03-04T10:02:36Z-
dc.date.available2008-03-04T10:02:36Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 329 - 333en
dc.identifier.urihttp://hdl.handle.net/2248/2118-
dc.description.abstractThis thesis is based on studies of two classical novae - V1425 Aquilae (J H K photometry and optical spectroscopy) and V723 Cassiopeiae (J H K photometry) and a sample of symbiotic stars (J H K photometry and Circular Variable Filter spectroscopy). The infrared data have been obtained from Mt. Abu IR Observatory of Physical Research Laboratory, Ahmedabad, and the optical spectra from Vainu Bappu Observatory of Indian Insitute of Astrophysics, Bangalore.en
dc.format.extent326895 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..329Ken
dc.subjectVariable starsen
dc.subjectNovaeen
dc.subjectSymbiotic;Photometryen
dc.subjectInfrared; Spectroscipyen
dc.subjectOpticalen
dc.titleStudies of classical novae and related objectsen
dc.typeArticleen
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