96 citations · 597 across the 15 of their papers we have counts for
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Dusty disk winds at the sublimation rim of the highly inclined, low mass YSO SU Aurigae
Aaron Labdon, Stefan Kraus, Claire L Davies +11
T Tauri stars are low-mass young stars whose disks provide the setting for planet formation. Despite this, their structure is poorly understood. We present new infrared interferome…
Protoplanetary Disk Masses from Radiative Transfer Modeling: A Case Study in Taurus
Nicholas P. Ballering, Josh A. Eisner
Measuring the masses of protoplanetary disks is crucial for understanding their planet-forming potential. Typically, dust masses are derived from (sub-)millimeter flux density meas…
High Precision Dynamical Masses of Pre-Main Sequence Stars with ALMA and Gaia
Patrick D. Sheehan, Ya-Lin Wu, Josh A. Eisner +1
The Keplerian rotation in protoplanetary disks can be used to robustly measure stellar masses at very high precision if the source distance is known. We present Atacama Large Milli…