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.
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页数：2
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