Response to Comment on “A noninteracting low-mass black hole–giant star binary system”

doi:10.1126/science.aba4356

GSTDTAP > 气候变化

DOI	10.1126/science.aba4356
	Response to Comment on “A noninteracting low-mass black hole–giant star binary system”
	Todd A. Thompson; Christopher S. Kochanek; Krzysztof Z. Stanek; Carles Badenes; Tharindu Jayasinghe; Jamie Tayar; Jennifer A. Johnson; Thomas W.-S. Holoien; Katie Auchettl; Kevin Covey
	2020-05-08
发表期刊	Science
出版年	2020
英文摘要	Van den Heuvel and Tauris argue that if the red giant star in the system 2MASS J05215658+4359220 has a mass of 1 solar mass ( M ☉), then its unseen companion could be a binary composed of two 0.9 M ☉ stars, making a triple system. We contend that the existing data are most consistent with a giant of mass 3.2−1.0+1.0 M ☉, implying a black hole companion of 3.3−0.7+2.8 M ☉.
领域	气候变化 ; 资源环境
URL	查看原文
引用统计
文献类型	期刊论文
条目标识符	http://119.78.100.173/C666/handle/2XK7JSWQ/249837
专题	气候变化资源环境科学
推荐引用方式 GB/T 7714	Todd A. Thompson,Christopher S. Kochanek,Krzysztof Z. Stanek,等. Response to Comment on “A noninteracting low-mass black hole–giant star binary system”[J]. Science,2020.
APA	Todd A. Thompson.,Christopher S. Kochanek.,Krzysztof Z. Stanek.,Carles Badenes.,Tharindu Jayasinghe.,...&Kevin Covey.(2020).Response to Comment on “A noninteracting low-mass black hole–giant star binary system”.Science.
MLA	Todd A. Thompson,et al."Response to Comment on “A noninteracting low-mass black hole–giant star binary system”".Science (2020).