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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3228
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dc.contributor.authorAnupama, G. C-
dc.date.accessioned2008-08-22T05:27:55Z-
dc.date.available2008-08-22T05:27:55Z-
dc.date.issued1997-11-
dc.identifier.citationAstronomical Journal, Vol.114, No. 5, pp. 2054 - 2057en
dc.identifier.issn0004-6256-
dc.identifier.urihttp://hdl.handle.net/2248/3228-
dc.description.abstractOptical spectra of three recent supernovae of type Ia: SN1995al in NGC 3021, SN1997Y in NGC 4675, and SN 1997bp in NGC 4680 are presented. Comparing the spectra with those of other normal type a supernovae, the epoch since maximum is estimated for each of the supernovae. Based on the blueshift of the Si II 6355 Å feature, and its location in the galaxy, it appears that Sn 1997 belongs to the older, bulge population of the galaxy.en
dc.format.extent473447 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997AJ....114.2054Aen
dc.subjectSupernovae: Individual: SN 1995ALen
dc.subjectSupernovae: Individual: SN1997Yen
dc.subjectSupernovae: Individual: SN 1997BPen
dc.titleOptical Spectra of Recent Supernovae of Type Ia: SN1995AL, SN1997Y, SN 1997BPen
dc.typeArticleen
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