NAOC Open IR
Self-microlensing in compact binary systems
Qin B(秦波); Wu XP(武向平); Zou ZL(邹振隆)
1997
Source PublicationChinese Physics Letters
ISSN0256-307X
Volume14Issue:2Pages:155
AbstractThe signature of the self-microlensing in compact binaries (white dwarfs, neutron stars and black holes) is a flare with the characteristic time of typically a few minutes. The probability of detecting these microlensing events can be as high as 1/50 for a photometric accuracy of Delta m = 0.01 in magnitude. The discovery of the self-microlensing by binaries would furnish an additional way to find the masses of the lens and the companion, and will be promising for the searches of black holes.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/44304
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Qin B,Wu XP,Zou ZL. Self-microlensing in compact binary systems[J]. Chinese Physics Letters,1997,14(2):155.
APA 秦波,武向平,&邹振隆.(1997).Self-microlensing in compact binary systems.Chinese Physics Letters,14(2),155.
MLA 秦波,et al."Self-microlensing in compact binary systems".Chinese Physics Letters 14.2(1997):155.
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