Bulge Microlensing is a gravitational microlensing phenomenon in which the light from a background star in the Galactic Bulge is transiently magnified by the gravitational field of a foreground compact object, enabling the detection and study of dark or low-luminosity mass components within the Bulge region.
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Gravitational microlensing by double stars and planetary systems
Shunde Mao, B. Paczyński · The Astrophysical Journal · 1991 · 746 citations
Natural Sciences, Astronomy, Physics +12
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289
The Ohio State University
Columbus, United States
33 h-index
141 publications
7.2K citations
University of Canterbury
Christchurch, New Zealand
25 h-index
72 publications
6.3K citations
University of Warsaw
Warsaw, Poland
21 h-index
253 publications
11.6K citations
Nagoya University
Nagoya, Japan
20 h-index
174 publications
15K citations
Chungbuk National University
Cheongju-si, South Korea
20 h-index
35 publications
1.6K citations
University of Notre Dame
Notre Dame, United States
19 h-index
32 publications
3K citations
Korea Astronomy and Space Science Institute
Daejeon, South Korea
18 h-index
130 publications
5.7K citations
University of Auckland
Auckland, New Zealand
18 h-index
75 publications
7.1K citations
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ApJ · 80 publications · 7.6K citations
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- Astronomy and Astrophysics
16 publications · 676 citations
14
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- CERN Document Server (European Organization for Nuclear Research)
Repository · 9 publications · 445 citations
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- The Astronomical Journal
AJ · 8 publications · 254 citations
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