ABSTRACT. Explosive hydrogen burning in type I X-ray bursts (XRBs) is driven by charged particle reactions creating isotopes with masses up to A ~ 100. Since charged particle reactions in a stellar environment are very temperature sensitive, we use a realistic time-dependent general relativistic and self-consistent model of type I X-ray bursts to provide accurate values of the burst temperatures and densities. This allows a detailed and accurate time-dependent identification of the reaction flow from the surface layers through the convective region and the ignition region to the neutron star ocean. Using this, we determine the relative importance of specific nuclear reactions in the X-ray burst.

Subject headings: nuclear reactions, nucleosynthesis, abundances; stars: neutron; X-rays: bursts

Print publication: Issue 1 (2008 January)
Received 2007 March 13, accepted for publication 2007 June 22