Author/Authors :
J.L. Fisker، نويسنده , , E.F. Brown، نويسنده , , M. Liebend?rfer، نويسنده , , F.-K. Thielemann، نويسنده , , K. Langanke and M. Wiescher، نويسنده ,
Abstract :
This paper reports on the detailed rp-process reaction flow on an accreting neutron star and the resulting ashes of a type I X-ray burst. It is obtained by coupling a 298 isotope reaction network to a self-consistent one-dimensional model calculation with a constant accretion rate of View the MathML source.
