activity
20172026
most citedSelf-consistent ring model in protoplanetary disks: temperature dips and substructure formation

14 citations · 29 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.EP2026

Exoplanet System Architecture: Sculpting the Inner Regions

Mark R. Swain, Geoffrey Bryden, Jonathan C. Tan +14

In this study, we seek to improve our understanding of the competing roles of disk-driven and planet-planet dynamical migration in sculpting planetary system architecture in the in…

astro-ph.SR2026★ 1 cited

Modeling YSO Jets in 3D III: Dependence of Accretion and Jet Properties on Stellar Magnetospheric Field Strength and Rotation

Yisheng Tu, Zhi-Yun Li, Zhaohuan Zhu +1

Observations of Young Stellar Objects (YSOs) systems reveal a wide diversity of jet properties, from well-collimated bipolar jets to uni-polar jets and systems with no detectable j…

astro-ph.SR2025★ 2 cited

A tale of three tails: A misaligned streamer and mysterious structures around [BHB2007]1

Aashish Gupta, Antonio S. Hales, L. Ilsedore Cleeves +8

Recent discoveries of streamer-like structures around protostellar sources challenge the traditional picture of isolated, axisymmetric star formation. Here, we present new ALMA obs…

astro-ph.EP2025★ 4 cited

Hydrodynamical Simulations of Planet Rebound Migration in Photo-evaporating Disks

Beibei Liu, Clément Baruteau, Zhaohuan Zhu +2

This study investigates the orbital migration of a planet located near the truncated edge of protoplanetary disks, induced by X-ray photo-evaporation originating from the central s…

astro-ph.SR2025★ 1 cited

The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars

Caeley V. Pittman, C. C. Espaillat, Zhaohuan Zhu +4

Classical T Tauri stars (CTTS) exhibit strong variability over timescales of minutes to decades. However, much theoretical work assumes that CTTS are in stable spin states. Here, w…

astro-ph.SR2025

The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars

Caeley V. Pittman, C. C. Espaillat, Connor E. Robinson +20

Magnetospheric accretion is a key process that shapes the inner disks of T Tauri stars, controlling mass and angular momentum evolution. It produces strong ultraviolet and optical…