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20242026
most citedEvidence for Variable Accretion onto PDS 70 c and Implications for Protoplanet Detections

17 citations · 20 across the 16 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2026

Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence

Ezequiel Manzo-Martínez, Ramiro Franco-Hernández, Nuria Calvet +3

We present a new approach to calculate the geometry and emission of the dust inner wall in disks around T Tauri stars. This calculation follows a self-consistent approach given the…

astro-ph.SR2026

Understanding Balmer Decrements in T Tauri stars in terms of Multiflow Magnetospheric Accretion

Naiara Patiño, Nuria Calvet, Gladis Magris +4

Magnetospheric accretion is the paradigm for accretion in Classical T-Tauri Stars (CTTS). However, the standard, one-flow magnetospheric accretion model fails to replicate importan…

astro-ph.SR2026

AREPAS: A Resource for Exploring Protostellar Accretion Systems - Data Release I

Marbely Micolta, Thanawuth Thanathibodee, Katya Gozman +1

We present AREPAS, a visualization tool for the exploration of the first data release of the open library of magnetospheric accretion models for T Tauri Stars. The dataset covers t…

astro-ph.SR2026

Accretion onto the Embedded Protostar L1527 IRS: Insights from JWST NIRSpec and MIRI Observations

W. Blake Drechsler, John J. Tobin, Patrick D. Sheehan +12

Accretion is the primary driver of protostellar evolution, regulating mass assembly and shaping the physical and chemical environments of young stellar objects. Quantifying accreti…

astro-ph.SR2025★ 1 cited

IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

Dan M. Watson, Mayank Narang, Caeley V. Pittman +41

The earliest stages of star formation are highlighted by complex interactions between accretion, outflow, and radiative processes, which shape the chemical and physical environment…

astro-ph.SR2025

The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection

Caeley V. Pittman, Catherine C. Espaillat, Thanawuth Thanathibodee +3

The properties of stars and planets are shaped by the initial conditions of their natal clouds. However, the spatial scales over which the initial conditions can exert a significan…