3 citations · 7 across the 10 of their papers we have counts for
10 papers
An Adolescent and Near-Resonant Planetary System Near the End of Photoevaporation
Mu-Tian Wang, Fei Dai, Hui-Gen Liu +28
Young exoplanets provide vital insights into the early dynamical and atmospheric evolution of planetary systems. Many multi-planet systems younger than 100 Myr exhibit mean-motion…
Testing the Origin of Hot Jupiters with Atmospheric Surveys
Lina D'Aoust, Ben Coull-Neveu, Eve J. Lee +1
In spite of their long detection history, the origin of hot Jupiters remains to be resolved. While multiple dynamical evidence suggests high-eccentricity migration is most likely,…
Resolving the Super-Earth/Gas Giant Connection in Stellar Mass and Metallicity
Marta L. Bryan, Eve J. Lee
The observed correlation between inner super-Earths and outer gas giants places strong constraints on formation theories. Building on previous work, Bryan Lee 2024 showed that…
Carving the Edges of the Rocky Planet Population
Eve J. Lee, James E. Owen
Short-period planets provide ideal laboratories for testing star-planet interaction. Planets that are smaller than 2 are considered to be largely rocky either havin…
Planet Mass Function around M stars at 1-10 au: A Plethora of sub-Earth mass objects
Yayaati Chachan, Eve J. Lee
Small planets ( M) at intermediate orbital distances (1 au) represent an uncharted territory in exoplanetary science. The upcoming microlensing survey by…
Impacting Atmospheres: How Late-Stage Pollution Alters Exoplanet Composition
Emilia Vlahos, Yayaati Chachan, Vincent Savignac +1
Atmospheric composition of exoplanets is often considered as a probe of the planet's formation condition. How exactly the initial chemical memory may be altered from the birth to t…
On the Formation of Planets in the Milky Way's Thick Disk
Tim Hallatt, Eve J. Lee
Exoplanet demographic surveys have revealed that close-in (1 au) small planets orbiting stars in the Milky Way's thick disk are less abundant than those or…
The First Evidence of a Host Star Metallicity Cut-off In The Formation of Super-Earth Planets
Kiersten M. Boley, Jessie L. Christiansen, Jon Zink +7
Planet formation is expected to be severely limited in disks of low metallicity, owing to both the small solid mass reservoir and the low opacity accelerating the disk gas dissipat…
Giant Outer Transiting Exoplanet Mass (GOT `EM) Survey. V. Two Giant Planets in Kepler-511 but Only One Ran Away
Yayaati Chachan, Paul A. Dalba, Daniel P. Thorngren +6
Systems hosting multiple giant planets are important laboratories for understanding planetary formation and migration processes. We present a nearly decade-long Doppler spectroscop…
The Not-So Dramatic Effect of Advective Flows on Gas Accretion
Vincent Savignac, Eve J. Lee
Super-Earths and mini-Neptunes are the most common types of exoplanets discovered, yet the physics of their formation are still debated. Standard core accretion models in gas-rich…