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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1837
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dc.contributor.authorKamath, U. S-
dc.contributor.authorAshok, N. M-
dc.contributor.authorChandrasekhar, T-
dc.date.accessioned2007-09-27T11:14:41Z-
dc.date.available2007-09-27T11:14:41Z-
dc.date.issued1996-
dc.identifier.citationBASI, Vol.24 No. 4 pp. 683-686en
dc.identifier.urihttp://hdl.handle.net/2248/1837-
dc.description.abstractJHK photometry of the slow, Fe-II type nova- Nova Aquilae 1995- obtained at the 1.2m Gurushikhar Infrared Telescope (GIRT) is presented here. Evidence for the presence of dust in the nova ejected based on these observations is discussed.en
dc.format.extent179965 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996BASI...24..683Ken
dc.subjectNova Aquliaeen
dc.subjectinfrared observationsen
dc.titleNear-infrared observations of nova Aquilae 1995en
dc.typeArticleen
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