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Abstract
The Galactic bulge source MOA-2010-BLG-523S exhibited short-term deviations from a standard microlensing light curve near the peak of an A(max) similar to 265 high-magnification microlensing event. The deviations originally seemed consistent with expectations for a planetary companion to the principal lens. We combine long-term photometric monitoring with a previously published high-resolution spectrum taken near peak to demonstrate that this is an RS CVn variable, so that planetary microlensing is not required to explain the light-curve deviations. This is the first spectroscopically confirmed RS CVn star discovered in the Galactic bulge.
Original language | English |
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Article number | 141 |
Number of pages | 11 |
Journal | Astrophysical Journal |
Volume | 763 |
Issue number | 2 |
DOIs | |
Publication status | Published - 1 Feb 2013 |
Keywords
- Gravitational lensing: micro
- Planetary systems
- Starspots
- Stars: variables: general
- Gravitational lensing experiment
- Galactic bulge
- Microlensing events
- High-magnification
- Variable-stars
- Dwarf stars
- Systems
- Photometry
- Rotation
- Catalog
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Dive into the research topics of 'MOA-2010-BLG-523: "Failed Planet" = RS CVn Star'. Together they form a unique fingerprint.Projects
- 1 Finished
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Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014
Horne, K. D. (PI)
Science & Technology Facilities Council
1/10/11 → 31/03/12
Project: Standard