A CONTINUUM OF PLANET FORMATION BETWEEN 1 AND 4 EARTH RADII
It has long been known that stars with high metallicity are more likely to host giant planets than stars with low metallicity. Yet the connection between host star metallicity and the properties of small planets is only just beginning to be investigated. It has recently been argued that the metallic...
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| Format: | Article |
| Language: | en_US |
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Institute of Physics/American Astronomical Society
2015
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| Online Access: | http://hdl.handle.net/1721.1/96713 https://orcid.org/0000-0001-5761-6779 |