Elemental abundances in CEMP stars: r– and s–process elements

Goswami, A; Athiray, S. P; Drisya, K

Home
→
IIAP Publications
→
IIAP Publications
→
View Item

dc.contributor.author	Goswami, A
dc.contributor.author	Athiray, S. P
dc.contributor.author	Drisya, K
dc.date.accessioned	2010-08-20T11:16:27Z
dc.date.available	2010-08-20T11:16:27Z
dc.date.issued	2010
dc.identifier.citation	Chaudhuri, R. K., Mekkaden, M. V., Raveendran, A. V & Narayanan, A. S., eds., Recent Advances In Spectroscopy: Theoretical, Astrophysical And Experimental Perspectives, Proceedings of the International Conference on Recent Advances in Spectroscopy - Theoretical, Astrophysical and Experimental Perspectives, Jan 28-31, 2009, Indian Institute of Astrophysics, Kodaikanal Observatory, Bangalore, India, pp. 211-216	en
dc.identifier.uri	http://hdl.handle.net/2248/5226
dc.description	The original publication is available at springerlink.com	en
dc.description.abstract	A number of Carbon-Enhanced Metal-poor (CEMP) stars are known to exhibit enhancement of both r – and s – process elements. An understanding of the relative contributions from r – and s – process would provide insight into the production mechanisms, nucleosynthetic sites and origins of the heavy elements observed in the stars. We have investigated ways to delineate the observed abundances into their respective r – and s – process contributions. Preliminary results obtained using appropriate model functions in the framework of a parametric model are discussed.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.ispartofseries	Astrophysics and Space Science Proceedings
dc.relation.uri	http://www.springerlink.com/content/n2v87n6j20810162/	en
dc.rights	© Springer	en
dc.title	Elemental abundances in CEMP stars: r– and s–process elements	en
dc.type	Article	en