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Gravitational microlensing: results and perspectives in brief

2006/10/29 by A. F. Zakharov, Alexander F. Zakharov, Zakharov, Alexander F.
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #History and Developments in Astronomy #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0610857

8 pages, 1 figure, An invited lecture at the Helmholtz International Summer School "Dense Matter in Heavy Ion Collisions and Astrophysics", Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, Russia, August 21 - September 1, 2006, added reference, corrected misprint

openalex publication_date 2006/10/29 · arxiv created 2006/11/23 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Basics of standard theory of microlensing are introduced. Results of microlensing observations toward Magellanic Clouds and relations with dark matter (DM) problem in our Galaxy are described. Pixel microlensing observations and recent discoveries of planets with microlensing observations are listed.

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