Supernova induced star formation

dc.contributor.author	Ramadurai, S
dc.date.accessioned	2006-04-10T09:24:36Z
dc.date.available	2006-04-10T09:24:36Z
dc.date.issued	1986-12
dc.identifier.citation	BASI, Vol. 14, No. 4, pp. 207-210	en
dc.identifier.uri	http://hdl.handle.net/2248/918
dc.description.abstract	The 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 history	en
dc.format.extent	351364 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Star formation	en
dc.subject	Supernova	en
dc.subject	Explosive nucleosynthesis	en
dc.title	Supernova induced star formation	en
dc.type	Article	en