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.
|Number of pages||4|
|Journal||Nuclear Physics A|
|Publication status||Published - 21 May 2001|
|Event||6th International Conference on Nuclei in the Cosmos - AARHUS, Denmark|
Duration: 27 Jun 2000 → 1 Jul 2000