Limits on compact halo objects as dark matter from gravitational microlensing

被引：0

作者：

Jetzer, Philippe ^{[1
]}

机构：

[1] Univ Zurich, Inst Theoret Phys, CH-8057 Zurich, Switzerland

来源：

1ST INTERNATIONAL CONFERENCE ON NEW FRONTIERS IN PHYSICS | 2014年 / 70卷

关键词：

LARGE-MAGELLANIC-CLOUD; OPTICAL DEPTH; OGLE-II; BULGE; EVENT; M31; LMC; CONSTRAINTS; TELESCOPE; MACHOS;

D O I：

10.1051/epjconf/20147000025

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Microlensing started with the seminal paper by Paczyfiski in 1986 [1], first with observations towards the Large Magellanic Cloud and the galactic bulge. Since then many other targets have been observed and new applications have been found. In particular, it turned out to be a powerful method to detect planets in our galaxy and even in the nearby M31. Here, we will present some results obtained so far by microlensing without being, however, exhaustive.

引用

页数：10

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