activity
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

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2021★ 10 cited

A Deep Search for Five Molecules in the 49 Ceti Debris Disk

Jessica Klusmeyer, A. Meredith Hughes, Luca Matra +9

Surprisingly strong CO emission has been observed from more than a dozen debris disks around nearby main-sequence stars. The origin of this CO is unclear, in particular whether it…

astro-ph.SR2021★ 4 cited

The first radio spectrum of a rapidly rotating A-type star

Jacob Aaron White, F. Tapia-Vázquez, A. G. Hughes +9

The radio spectra of main-sequence stars remain largely unconstrained due to the lack of observational data to inform stellar atmosphere models. As such, the dominant emission mech…

astro-ph.SR2020★ 10 cited

The MESAS Project: ALMA observations of the F-type stars Lep, Vir A, and Vir B

Jacob Aaron White, F. Tapia-Vázquez, A. G. Hughes +7

The spectrum of stars in the submillimeter to centimeter wavelength range remains poorly constrained due to a lack of data for most spectral types. An accurate characterization of…

astro-ph.SR2019

Variability in the Assembly of Protostellar Systems

Joel D. Green, Yao-Lun Yang, Tom Megeath +17

Understanding the collapse of clouds and the formation of protoplanetary disks is essential to understanding the formation of stars and planets. Infall and accretion, the mass-aggr…

astro-ph.SR2019★ 9 cited

The MESAS Project: Long wavelength follow-up observations of Sirius A

Jacob Aaron White, Jason Aufdenberg, Aaron C. Boley +13

Modeling the submillimeter to centimeter emission of stars is challenging due to a lack of sensitive observations at these long wavelengths. We launched an ongoing campaign to obta…

astro-ph.SR2018

Science with an ngVLA: Stellar Emission as a Source of Flux Bias in Debris Disks

Jacob Aaron White, Jason Aufdenberg, Aaron C. Boley +5

Our understanding of stellar atmospheres and our ability to infer architectures of extrasolar planetary systems rely on understanding the emission of stars at submillimeter to cent…