Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/754
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dc.contributor.authorBanerjee, D. P. K-
dc.date.accessioned2006-03-14T05:03:33Z-
dc.date.available2006-03-14T05:03:33Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 81-86en
dc.identifier.urihttp://hdl.handle.net/2248 /754-
dc.description.abstractWe discuss our recent observations of the interesting but enigmatic nova-like variable V4332 Sgr. The object shows a remarkably rich near-infrared and optical spectrum with several unusual spectral features generally not seen in classical novae. Our results support the emerging consensus that V4332 Sgr, and its possible analog V838 Mon, constitute a new class of eruptive variables. Our results indicate that a cold circumstellar disc containing gas, dust and water ice surrounds the object. Though the cause of the outburst in these objects is not completely understood, we propose a plausible planetary-capture scenario to explain the eruption of V4332 Sgren
dc.format.extent233758 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectV4332 Sgren
dc.subjectnovaeen
dc.subjectInfra-red spectroscopyen
dc.subjectCOen
dc.subjectAlOen
dc.subjectwater iceen
dc.titleStudies of the peculiar nova V4332 Sgren
dc.typeArticleen
Appears in Collections:BASI Publications

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