activity
20022025
most citedEvidence for a developing gap in a 10 Myr old protoplanetary disk

560 citations · 7.1k across the 88 of their papers we have counts for

collaborators

88 papers

astro-ph.SR2025★ 4 cited

The Dynamic Inner Disk of a Planet Forming Star

Benjamin R. Setterholm, John D. Monnier, Fabien Baron +13

Planets are a natural byproduct of the stellar formation process, resulting from local aggregations of material within the disks surrounding young stars. Whereas signatures of gas-…

astro-ph.SR2023★ 1 cited

Twenty-Five Years of Accretion onto the Classical T Tauri Star TW Hya

Gregory J. Herczeg, Yuguang Chen, Jean-Francois Donati +39

Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time…

astro-ph.SR2023

The Ca II lines as tracers of disk structure in T Tauri Stars: The Chamaeleon I region

Marbely Micolta, Nuria Calvet, Thanawuth Thanathibodee +4

We present a study of the Ca II K and IR-triplet lines in a sample of Classical T Tauri stars in the Chamaeleon I star-forming region. We study X-shooter spectra of the stars in th…

astro-ph.SR2023★ 1 cited

Constraints on star formation in Orion A from Gaia

Jairo A. Alzate, Gustavo Bruzual, Marina Kounkel +4

We develop statistical methods within a Bayesian framework to infer the star formation history from photometric surveys of pre-main sequence populations. Our procedures include cor…

astro-ph.SR2023★ 4 cited

Strong Variability in AzV 493, an Extreme Oe-Type Star in the SMC

M. S. Oey, N. Castro, M. Renzo +11

We present 18 years of OGLE photometry together with spectra obtained over 12 years, revealing that the early Oe star AzV 493 shows strong photometric (Delta I < 1.2 mag) and spect…

astro-ph.SR2022★ 22 cited

A Census of the Low Accretors. II: Accretion Properties

Thanawuth Thanathibodee, Brandon Molina, Javier Serna +4

Much is known about the processes driving accretion from protoplanetary disks onto low-mass pre-main-sequence stars (T Tauri stars). Nevertheless, it is unclear how accretion stops…