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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/918
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dc.contributor.authorRamadurai, S-
dc.date.accessioned2006-04-10T09:24:36Z-
dc.date.available2006-04-10T09:24:36Z-
dc.date.issued1986-12-
dc.identifier.citationBASI, Vol. 14, No. 4, pp. 207-210en
dc.identifier.urihttp://hdl.handle.net/2248/918-
dc.description.abstractThe evidence for the triggering of star formation by shocks from expanding supernova shells is examined with special emphasis on the solar system. It is shown that the recently discovered isotopic anomalies, mainly in Ti, can serve as the best signature for this purpose. It is suggested that the discovery of correlated anomalies in Ti, Fe, and Ca will give important clues to the nucleosynthetic origin, as well as to the chemical historyen
dc.format.extent351364 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStar formationen
dc.subjectSupernovaen
dc.subjectExplosive nucleosynthesisen
dc.titleSupernova induced star formationen
dc.typeArticleen
Appears in Collections:BASI Publications

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