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20092024
most citedEarly Planet Formation in Embedded Disks (eDisk). I. Overview of the Program and First Results

159 citations · 1.4k across the 46 of their papers we have counts for

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23 papers · 1 filter

astro-ph.SR2022★ 27 cited

ALMA Observations of the HD~110058 debris disk

Antonio S. Hales, SebastiÁn Marino, Patrick D. Sheehan +7

We present Atacama Large Millimeter Array (ALMA) observations of the young, gas-rich debris disk around HD110058 at 0.3-0.6\arcsec resolution. The disk is detected in the 0.85 and…

astro-ph.SR2022★ 24 cited

300: An ACA 870 m Continuum Survey of Orion Protostars and their Evolution

Samuel Federman, S. Thomas Megeath, John J. Tobin +11

We present an 870 m continuum survey of 300 protostars from the Herschel Orion Protostar Survey using the Atacama Compact Array (ACA). These data measure protostellar flux densi…

astro-ph.SR2022

A VLA View of the Flared, Asymmetric Disk Around the Class 0 Protostar L1527 IRS

Patrick D. Sheehan, John J. Tobin, Zhi-Yun Li +21

We present high resolution Karl G. Jansky Very Large Array (VLA) observations of the protostar L1527 IRS at 7 mm, 1.3 cm, and 2 cm wavelengths. We detect the edge-on dust disk at a…

astro-ph.SR2022

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars VI. Insights from Radiative Transfer Modeling

Patrick D. Sheehan, John J. Tobin, Leslie L. Looney +1

We present Markov Chain Monte Carlo radiative transfer modeling of a joint ALMA 345 GHz and spectral energy distribution dataset for a sample of 97 protostellar disks from the VLA…

astro-ph.SR2022★ 42 cited

The Rate, Amplitude and Duration of Outbursts from Class 0 Protostars in Orion

W. Zakri, S. T. Megeath, W. J. Fischer +18

At least half of a protostar's mass is accreted in the Class 0 phase, when the central protostar is deeply embedded in a dense, infalling envelope. We present the first systematic…

astro-ph.SR2020

Dynamical Masses of Young Stars Inferred from Two Transitions of CO with ALMA

Pranav H. Premnath, Ya-Lin Wu, Brendan P. Bowler +1

Stellar masses are fundamental but often difficult to measure. Thanks to the Atacama Large Millimeter Array (ALMA) and , dynamical masses of pre-main sequence stars can be pr…