Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2412
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dc.contributor.authorAshok, N. M-
dc.contributor.authorBanerjee, D. P. K-
dc.date.accessioned2008-06-06T06:59:00Z-
dc.date.available2008-06-06T06:59:00Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 343 - 344en
dc.identifier.urihttp://hdl.handle.net/2248/2412-
dc.description.abstractNear-IR spectroscopic observations are reported for the enigmatic, nova-like, variable V445 Puppis. The near-IR spectra are hydrogen-deficient and unusually rich in CI lines. The spectra indicate that the object could be a rare Helium nova. 16en
dc.format.extent55684 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..343Aen
dc.subjectSpectroscopyen
dc.subjectV445 Puppisen
dc.titleJHK Spectroscopy of the Enigmatic Variable V445 Puppisen
dc.typeArticleen
Appears in Collections:BASI Publications

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