Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4270
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dc.contributor.authorKochhar, R. K-
dc.contributor.authorPrabhu, T. P-
dc.date.accessioned2009-01-16T14:24:39Z-
dc.date.available2009-01-16T14:24:39Z-
dc.date.issued1984-03-
dc.identifier.citationAstrophysics and Space Science, Vol. 100, No. 1 - 2, pp. 369 - 379en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4270-
dc.description.abstractIt is shown that there is a correlation between the occurrence of supernovae and nuclear activity in elliptical galaxies. Both shun a canonical elliptical, and occur only in those ellipticals which accrete gas. It is also shown that the hypothesis that all SNI come from short lived stars is consistent with the color observations of elliptical galaxies. It is proposed that there is a class of intrisically rounder, massive, dusty, metal-rich ellipticals which produce supernovae and are more likely to contain a radio source.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS.100..369Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF00651612en
dc.rights© D. Reidel Publishing Co.en
dc.subjectElliptical Galaxiesen
dc.subjectNuclear Interactionsen
dc.subjectStellar Evolutionen
dc.subjectSupernovaeen
dc.subjectGalactic Nucleien
dc.subjectMass To Light Ratiosen
dc.subjectMetallicityen
dc.subjectRadio Galaxiesen
dc.subjectStellar Mass Accretionen
dc.titleOn the correlation between supernova occurrence and nuclear activity in elliptical galaxiesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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