We summarize the results of two experiments to address important issues related to the correlation between planet frequencies and properties and the metallicity of the hosts. Our results can usefully inform formation, structural, and evolutionary models of gas giant planets.
|Original language||English (US)|
|Number of pages||2|
|Journal||Proceedings of the International Astronomical Union|
|State||Published - Oct 2007|
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science