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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1171
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dc.contributor.authorAnupama, G. C-
dc.contributor.authorDuerbeck, H. W-
dc.contributor.authorPrabhu, T. P-
dc.contributor.authorJain, S. K-
dc.date.accessioned2006-07-18T05:34:04Z-
dc.date.available2006-07-18T05:34:04Z-
dc.date.issued1992-09-
dc.identifier.citationAstronomy and Astrophysics, Vol. 263, No. 1 - 2, pp. 87 – 96en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/1171-
dc.description.abstractSpectroscopy of the moderately fast nova V443 is presented. Observations were made during the brightness fluctuations following maximum and during the transition stage. A few broadband polarimetric observations are also given. The spectrum and its evolution are similar to novae with the same type of light curves. The extinction E(B-V) = 0.4 is derived from ratios of higher members of the hydrogen Balmer and Paschen series; a distance of 8.0 kpc is estimated from magnitude-decay time relations. Balmer line fluxes at late stages are used to derive the mass of the ejected ionized shell, about 3.5 x 10 exp -5 solar masses.en
dc.format.extent388283 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992A%26A...263...87A-
dc.subjectNovaeen
dc.subjectStellar Evolutionen
dc.subjectStellar Spectraen
dc.subjectAstronomical Polarimetry-
dc.subjectBalmer Series-
dc.subjectInterstellar Extinction-
dc.subjectLight Curve-
dc.subjectStellar Envelopes-
dc.subjectStellar Spectrophotometry-
dc.titleSpectral evolution of nova V443 Scuti 1989en
dc.typeArticleen
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