A Search for Unbound Stellar Companions to Pulsar J1124-5916

被引：5
|
作者：
Kochanek, C. S. [1 ,2 ]
机构：
[1] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA
[2] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, 191 W Woodruff Ave, Columbus, OH 43210 USA
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2023年 / 519卷 / 03期
关键词：
stars: massive; supernovae:general; supernovae; SUPERNOVA REMNANT G292.0+1.8; PSR J1124-5916; WIND NEBULA; MASS; EVOLUTION; BINARIES; DISCOVERY; EJECTA; RADIO; STARS;
D O I：
10.1093/mnras/stac2616
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We searched for and found no higher mass (>(similar to)3M(?)) unbound binary stellar companions to the progenitor of pulsar J1124-5916. There are lower mass candidates, but they all have high probabilities of being false positives. There are no candidates for it now being a fully unbound triple system. Even if one of the lower mass candidates is an unbound companion, it seems unlikely that it could have contributed to stripping the progenitor prior to the supernova. The stars are too low mass to be significant mass gainers, and they are too slowly moving to be the survivors of a compact, post-common envelope binary. The addition of one more system slightly improves the statistical constraints on the binary and triple status of supernova progenitors just before and after death.
引用
收藏
页码：3865 / 3871
页数：7
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