| 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 (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
