The High Albedo of the Hot Jupiter Kepler-7 B
Hot Jupiters are expected to be dark from both observations (albedo upper limits) and theory (alkali metals and/or TiO and VO absorption). However, only a handful of hot Jupiters have been observed with high enough photometric precision at visible wavelengths to investigate these expectations. The N...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
IOP Publishing
2012
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| Online Access: | http://hdl.handle.net/1721.1/74166 https://orcid.org/0000-0002-6892-6948 |