Comment on "A noninteracting low-mass black hole-giant star binary system"

被引：30

作者：

van den Heuvel, Ed P. J. ^{[1
]}

Tauris, Thomas M. ^{[2
,3
]}

机构：

[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 XH Amsterdam, Netherlands

[2] Aarhus Univ, Aarhus Inst Adv Studies, DK-8000 Aarhus C, Denmark

[3] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark

来源：

SCIENCE | 2020年 / 368卷 / 6491期

基金：

欧盟地平线“2020”;

关键词：

TRIPLE; MODEL; WIND;

D O I：

10.1126/science.aba3282

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Thompson et al. (Reports, 1 November 2019, p. 637) interpreted the unseen companion of the red giant star 2MASS J05215658+4359220 as most likely a black hole. We argue that if the red giant's mass is similar to 1 solar mass, its companion can be a close binary consisting of two main-sequence stars. This would explain why no x-ray emission is detected from the system.

引用

页数：2

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