dc.contributor.author |
Goswami, A |
|
dc.date.accessioned |
2012-07-12T14:36:15Z |
|
dc.date.available |
2012-07-12T14:36:15Z |
|
dc.date.issued |
2011 |
|
dc.identifier.citation |
ASI Conference Series, Vol. 3, pp. 45-48 |
en |
dc.identifier.isbn |
978-81-922926-1-8 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5794 |
|
dc.description |
Open Access |
en |
dc.description.abstract |
The chemical composition of stars belonging to the halo and the disk of our Galaxy as well as a few nearby galaxies are the primary sources of our understanding of the Galactic Chemical Evolution (GCE). The abundance trends implied by the abundance ratios of the chemical elements as a function of time and metallicity trace the chemical history of our Galaxy which could be understood in the framework of a Galactic Chemical Evolution Model (GCEM). Among the basic ingredients of a GCEM `stellar yields' play an important role as they implicitly contain a physical scenario of stellar nucleosynthesis and evolution. Improved input along with a realistic model of chemical evolution are expected to result better simulation of the observed abundances. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2011ASInC...3...45G |
en |
dc.rights |
© Astronomical Society of India |
en |
dc.subject |
Stars: stellar yields |
en |
dc.subject |
Stars: abundances |
en |
dc.subject |
Stars: chemical evolution |
en |
dc.title |
Stellar yields and Galactic chemical evolution |
en |
dc.type |
Book chapter |
en |