Chemical evolution of intermediate mass nuclei in the solar neighbourhood and the halo of the galaxy

dc.contributor.author	Goswami, A
dc.contributor.author	Prantzos, N
dc.date.accessioned	2008-03-03T10:48:24Z
dc.date.available	2008-03-03T10:48:24Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 305 - 308	en
dc.identifier.uri	http://hdl.handle.net/2248/2110
dc.description.abstract	Recent observations of Fe group elements in very low metallicity stars show an evolutionary trend very different from that of Fe, implying divergent paths of chemical evolution for these elements. In the present work we have investigated the chemical evolution of intermediate mass nuclei in the solar neighbourhood and the halo of the Galaxy with a two zone model of Galactic chemical evolution using a comprehensive set of theoretically computed yields covering the entire range from H to Ge. It is shown that with a two zone model the main observational constraints of the solar neighbourhood can be satisfied.	en
dc.format.extent	335778 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..305G	en
dc.subject	Galaxy	en
dc.subject	Chemical evolution	en
dc.title	Chemical evolution of intermediate mass nuclei in the solar neighbourhood and the halo of the galaxy	en
dc.type	Article	en