The endpoint of the rp-process on accreting neutron stars

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.

Full text not available from this repository.

Official URL: http://edoc.unibas.ch/dok/A5839312

Downloads: Statistics Overview


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)
UniBasel Contributors:Rauscher, Thomas
Item Type:Article, refereed
Article Subtype:Research Article
Publisher:North Holland
Note:Publication type according to Uni Basel Research Database: Journal article
Identification Number:
Last Modified:14 Sep 2012 07:18
Deposited On:14 Sep 2012 06:44

Repository Staff Only: item control page