THE ORIGIN OF THE PLANET AROUND PSR-1829-10

被引:12
作者
NAKAMURA, T [1 ]
PIRAN, T [1 ]
机构
[1] HEBREW UNIV JERUSALEM,RACAH INST PHYS,JERUSALEM,ISRAEL
关键词
PLANETS; FORMATION; PULSARS; STARS; NEUTRON;
D O I
10.1086/186217
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider various scenarios for formation of a planet around a neutron star, as observed in PSR 1829-10. We show that matter, ablated from a companion 1.5 M. star which was orbiting around the neutron star progenitor at a distance of almost-equal-to 3 x 10(12) cm, would be captured by the neutron star and form a disk around it. The companion star escaped from the system during supernova event, and the observed planet was eventually formed from this disk.
引用
收藏
页码:L81 / L84
页数:4
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