activity
20242026
collaborators

7 papers

astro-ph.EP2026

Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned

Xian-Yu Wang, Songhu Wang

In this work, we show that warm sub-Saturns orbiting single stars are predominantly aligned, in contrast to hot sub-Saturns, which are frequently misaligned, with the two populatio…

astro-ph.EP2025

Planet Across Space and Time (PAST). VII. The origin and tidal evolution of hot Jupiters constrained by a broken age-frequency relation

Di-Chang Chen, Ji-Wei Xie, Ji-Lin Zhou +4

The discovery of hot Jupiters has challenged the classical planet formation theory. Although various formation mechanisms have been proposed, the dominant channel and relative cont…

astro-ph.EP2025

Early Evidence for Polar Orbits of Sub-Saturns Around Hot Stars

Emma Dugan, Xian-Yu Wang, Agustin Heron +4

Sub-Saturns have been reported to preferentially occupy near-polar orbits, but this conclusion has so far been based primarily on systems with cool host stars; obliquity measuremen…

astro-ph.EP2025

Migration and Evolution of giant ExoPlanets (MEEP) II: Super-Jupiters and Lithium-rich Host Stars

Jack Schulte, Joseph E. Rodriguez, David W. Latham +30

Although hot Jupiters were the first exoplanets discovered orbiting main sequence stars, the dominant mechanisms through which they form and evolve are not known. To address the qu…

astro-ph.EP2025

TOI-880 is an Aligned, Coplanar, Multi-planet System

Elina Y. Zhang, Huan-Yu Teng, Fei Dai +22

Although many cases of stellar spin-orbit misalignment are known, it is usually unclear whether a single planet's orbit was tilted or if the entire protoplanetary disk was misalign…

astro-ph.EP2024

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest Systems Exhibit Low Obliquities, Even around Hot Stars

Jace Rusznak, Xian-Yu Wang, Malena Rice +1

We present a pattern emerging from stellar obliquity measurements in single-star systems: planets with high planet-to-star mass ratios ( ) -- su…