Schatz, H. and Aprahamian, A. and Barnard, V. and Bildsten, L. and Cumming, A. and Ouellette, M. and Rauscher, T. and Thielemann, F. K. and Wiescher, M.. (2001) The endpoint of the rp-process on accreting neutron stars. Nuclear physics. A, Nuclear and hadronic physics, Vol. 688, H. 1-2 , S. 150C-153C.
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Official URL: http://edoc.unibas.ch/dok/A5839312
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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.
| Faculties and Departments: | 05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann) |
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| UniBasel Contributors: | Rauscher, Thomas |
| Item Type: | Article, refereed |
| Article Subtype: | Research Article |
| Publisher: | North Holland |
| ISSN: | 0375-9474 |
| Note: | Publication type according to Uni Basel Research Database: Journal article |
| Identification Number: |
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| Last Modified: | 14 Sep 2012 07:18 |
| Deposited On: | 14 Sep 2012 06:44 |
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