The endpoint of the rp-process on accreting neutron stars

dc.contributor.author	Schatz, H.
dc.contributor.author	Aprahamian, A.
dc.contributor.author	Bildsten, L.
dc.contributor.author	Cumming, A.
dc.contributor.author	Ouellette, M.
dc.contributor.author	Rauscher, T.
dc.contributor.author	Thielemann, Friedrich-Karl
dc.contributor.author	Wiescher, M.
dc.date.accessioned	2013-06-18T10:15:44Z
dc.date.available	2013-06-18T10:15:44Z
dc.date.issued	2001-05-21
dc.identifier.citation	Schatz , H , Aprahamian , A , Bildsten , L , Cumming , A , Ouellette , M , Rauscher , T , Thielemann , F-K & Wiescher , M 2001 , ' The endpoint of the rp-process on accreting neutron stars ' , Nuclear Physics A , vol. 688 , no. 1-2 , pp. 150C-153C .
dc.identifier.issn	0375-9474
dc.identifier.uri	http://hdl.handle.net/2299/10813
dc.description.abstract	We find that the rp process in X-ray bursts and in steady state burning, for example in X-ray pulsars, ends in a SnSbTe cycle. We discuss the consequences for the neutron star crust composition an X-ray burst light curves.	en
dc.format.extent	4
dc.language.iso	eng
dc.relation.ispartof	Nuclear Physics A
dc.subject	X-RAY-BURSTS
dc.title	The endpoint of the rp-process on accreting neutron stars	en
dc.contributor.institution	Centre for Astrophysics Research
dc.description.status	Peer reviewed
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true

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