Self-microlensing in compact binary systems
Qin B(秦波); Wu XP(武向平); Zou ZL(邹振隆)
Source PublicationChinese Physics Letters
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.
Document Type期刊论文
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.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[秦波]'s Articles
[武向平]'s Articles
[邹振隆]'s Articles
Baidu academic
Similar articles in Baidu academic
[秦波]'s Articles
[武向平]'s Articles
[邹振隆]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[秦波]'s Articles
[武向平]'s Articles
[邹振隆]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.