THE QUASI-STATIC EVOLUTION OF ONEMG CORES - EXPLOSIVE IGNITION DENSITIES AND THE COLLAPSE EXPLOSION ALTERNATIVE

被引:30
作者
CANAL, R [1 ]
ISERN, J [1 ]
LABAY, J [1 ]
机构
[1] CSIC,CTR ESTUDIS AVANCATS BLANES,E-17300 BLANES,SPAIN
关键词
STARS; INTERIORS; NEUTRON; WHITE DWARFS; SUPERNOVAE; GENERAL;
D O I
10.1086/186574
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The quasi-static evolution of an electron-degenerate ONeMg core is followed up to the point of explosive Ne-O ignition triggered by electron capture. Recently calculated electron-capture rates on Mg-24, Na-24, Ne-20, and F-20 are used, and the ignition density is found to be rho(ign) congruent-to 8.5 x 10(9) g cm-3 (when the Ledoux criterion for convection is adopted), instead of rho(ign) congruent-to 10(10) g cm-3 as in earlier calculations. Such a comparatively low ignition density should lead to complete explosive disruption of the core even if the thermonuclear burning propagated all the way as a conductive, laminar flame. The dependence of the ignition density on the treatment adopted for mixing in the semiconvective region and the astronomical implications of our results are briefly discussed.
引用
收藏
页码:L49 / L52
页数:4
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