The s-process in AGB stars

dc.contributor.author	Karakas, Amanda
dc.contributor.author	Lugaro, Maria
dc.coverage.spatial	Heidelberg Germany
dc.date.accessioned	2015-12-13T23:00:15Z
dc.date.created	July 19-23 2010
dc.date.issued	2010
dc.date.updated	2015-12-12T07:32:51Z
dc.description.abstract	About half of the solar abundances of elements heavier than iron are made by the slow neutron capture process (the s process) occurring in low and intermediate-mass asymptotic giant branch (AGB) stars. Elements are dredged from the core to the surface and
dc.identifier.uri	http://hdl.handle.net/1885/84037
dc.publisher	Conference Organising Committee
dc.relation.ispartofseries	11th Symposium on Nuclei in the Cosmos, NIC 2010
dc.source	Proceedings of Science
dc.title	The s-process in AGB stars
dc.type	Conference paper
local.bibliographicCitation.lastpage	10
local.bibliographicCitation.startpage	1
local.contributor.affiliation	Karakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliation	Lugaro, Maria, Monash University
local.contributor.authoruid	Karakas, Amanda, u4382192
local.description.embargo	2037-12-31
local.description.notes	Imported from ARIES
local.description.refereed	Yes
local.identifier.absfor	020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublication	f5625xPUB12302
local.identifier.scopusID	2-s2.0-84887449165
local.type.status	Published Version

Downloads

Now showing 1 - 1 of 1