论文标题
在近距离二进制中，低质量中子星的爆炸期间产生重元素
Production of Heavy Elements During the Explosion of a Low-Mass Neutron Star in a Close Binary
论文作者
论文摘要
在质量中，在质量中近不同的中子恒星的近距离二元二元二元二元的演变中，重元素的核合成被认为是质量的。与在文献中反复考虑的两个类似质量的中子星的合并相反，在最后阶段，这种二进制的演变包括快速向更大的恒星转移到更大的恒星和对低质量成分的爆炸性破坏。我们提供了爆炸的细节，并计算了各种初始条件中此过程中产生的重元素的丰度。
The nucleosynthesis of heavy elements in the scenario for the evolution of a close binary of neutron stars differing greatly in mass is considered. In contrast to the scenario for the merger of two neutron stars of comparable masses considered repeatedly in the literature, the evolution of such a binary at the final stage consists in a rapid mass transfer to the more massive star and an explosive disruption of the low-mass component. We provide the details of the explosion and calculate the abundances of the heavy elements produced in this process for various initial conditions.
