Polarimetry microlensing of close-in planetary systems
A close-in giant planetary (CGP) system has a net polarization signal whose value varies depending on the orbital phase of the planet. This polarization signal is either caused by the stellar occultation or by reflected starlight from the surface of the orbiting planet. When the CGP system is locate...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2017 April 5
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| In: |
The astrophysical journal
Year: 2017, Volume: 838, Issue: 2, Pages: 157 |
| ISSN: | 1538-4357 |
| DOI: | 10.3847/1538-4357/aa67e1 |
| Online Access: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.3847/1538-4357/aa67e1
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| Author Notes: | Sedighe Sajadian and Markus Hundertmark |
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Polarimetry microlensing of close-in planetary systems
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