Astrometric properties of gravitational binary-microlens events and their applications

被引:25
作者
Han, C [1 ]
Chu, M
Chang, K
机构
[1] Chungbuk Natl Univ, Dept Astron & Space Sci, Chongju 361763, South Korea
[2] Yonsei Univ, Dept Astron, Seoul 120749, South Korea
[3] Chungbuk Natl Univ, Dept Phys, Chongju 360764, South Korea
关键词
astrometry; binaries : general; gravitational lensing;
D O I
10.1086/307996
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we study the astrometric properties of gravitational microlensing events caused by binary lenses. By investigating the centroid shifts for various types of binary-lens events, we find that the deviations of the centroid shift trajectories from the elliptical ones of single-lens events are characterized by distortions, twistings, and big jumps. We study the conditions of binary-lens system configurations and source star trajectories for individual types of deviations. We find dramatic differences in the astrometric centroid shifts for binary-lens microlensing events that would be degenerate had their parameters been determined photometrically. Therefore, when additional astrometric observations of a binary-lens event are available, one can resolve the ambiguity of the binary-lens fit and uniquely determine the binary-lens parameters.
引用
收藏
页码:405 / 410
页数:6
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