Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3719
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dc.contributor.authorAnupama, G. C-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2008-09-17T12:19:47Z-
dc.date.available2008-09-17T12:19:47Z-
dc.date.issued1989-09-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 10, No. 3, pp. 237 - 255en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3719-
dc.description.abstractResults are reported from visual spectroscopy of the recurrent nova RS Oph, obtained with a Cassegrain spectrograph on the 102-cm reflector at Vainu Bappu Observatory in February-May 1985 (days 32-108 postoutburst). The data are presented in extensive tables and graphs and characterized in detail. It is estimated that the electron density in the ejected envelope decreased from 3 x 10 to the 9th/cu cm on day 32 to 1.8 x 10 to the 8th/cu cm on day 108; the temperature in the coronal line region decreased from 1.5 to 1.1 million K over the same period.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1989JApA...10..237Aen
dc.subjectLine spectraen
dc.subjectNovaeen
dc.subjectOptical emission spectroscopyen
dc.subjectStellar envelopesen
dc.subjectOphiuchi cloudsen
dc.subjectSpectrum analysisen
dc.subjectTables (data)en
dc.titleThe 1985 outburst of RS Ophiuchi - Spectroscopic resultsen
dc.typeArticleen
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