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20092022
most citedResolved Gas Interior to the Dust Rings of the HD 141569 Disk

31 citations · 192 across the 28 of their papers we have counts for

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astro-ph.EP2020★ 9 cited

ALMA and VLA Observations of EX Lupi in its Quiescent State

Jacob Aaron White, Á. Kóspál, A. G. Hughes +15

Extreme outbursts in young stars may be a common stage of pre-main-sequence stellar evolution. These outbursts, caused by enhanced accretion and accompanied by increased luminosity…

astro-ph.EP2019

Probing Unseen Planet Populations with Resolved Debris Disk Structures

Kate Su, Nick Ballering, Steve Ertel +10

Thousands of exoplanets have been found with many widely different from the ones in our own system. Despite the success, systems with planets in wide orbits analogous to those of J…

astro-ph.EP2019

Planet formation: The case for large efforts on the computational side

Wladimir Lyra, Thomas Haworth, Bertram Bitsch +54

Modern astronomy has finally been able to observe protoplanetary disks in reasonable resolution and detail, unveiling the processes happening during planet formation. These observe…

astro-ph.EP2018

Science with an ngVLA: Resolving the Radio Complexity of EXor and FUor-type Systems with the ngVLA

Jacob Aaron White, Marc Audard, Péter Ábrahám +17

Episodic accretion may be a common occurrence in the evolution of young pre-main sequence stars and has important implications for our understanding of star and planet formation. M…

astro-ph.EP2018★ 13 cited

Extended Millimeter Emission in the HD 141569 Circumstellar Disk Detected with ALMA

Jacob Aaron White, Aaron C. Boley

We present archival ALMA observations of the HD 141569 circumstellar disk at 345, 230, and 100 GHz. These data detect extended millimeter emission that is exterior to the inner dis…

astro-ph.EP2017★ 16 cited

ALMA and VLA Observations of the HD 141569 System

Jacob Aaron White, A. C. Boley, M. A. MacGregor +2

We present VLA 9 mm (33 GHz) observations of the HD 141569 system from semester 16A. The observations achieve a resolution of 0.25 arcsec ( au) and a sensitivity of $4.7~μ\…