28 citations · 95 across the 7 of their papers we have counts for
7 papers
Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+
Amina Diop, Kevin Flaherty, Chunhua Qi +7
Planets form in the midplanes of protoplanetary disks, thus investigating the properties of the midplane region can shed light on the physical and chemical processes governing the…
The influence of tight binaries on proto-planetary disk masses
Kevin Flaherty, Peter Knowlton, Tasan Smith-Gandy +5
Binary systems are a common site of planet formation, despite the destructive effects of the binary on the disk. While surveys of planet forming material have found diminished disk…
Revealing Fine Structure in Protoplanetary Disks with Physics Constrained Neural Fields
Aviad Levis, Nhan Luong, Richard Teague +3
Protoplanetary disks are the birthplaces of planets, and resolving their three-dimensional structure is key to understanding disk evolution. The unprecedented resolution of ALMA de…
Evidence for Non-zero Turbulence in the Protoplanetary disc around IM Lup
Kevin Flaherty, A. Meredith Hughes, Jacob B. Simon +6
The amount of turbulence in protoplanetary discs around young stars is critical for determining the efficiency, timeline, and outcomes of planet formation. It is also difficult to…
The Planet Formation Potential Around a 45 Myr old Accreting M Dwarf
Kevin M. Flaherty, A. Meredith Hughes, Eric E. Mamajek +1
Debris disk detections around M dwarfs are rare, and so far no gas emission has been detected from an M dwarf debris disk. This makes the 45 Myr old M dwarf WISEJ080822.18-644357.3…
A "Rosetta Stone" for protoplanetary disks: The synergy of multi-wavelength observations
A. Sicilia-Aguilar, A. Banzatti, A. Carmona +7
The recent progress in instrumentation and telescope development has brought us different ways to observe protoplanetary disks, including interferometers, space missions, adaptive…
Connecting X-ray and Infrared Variability among Young Stellar Objects: Ruling out potential sources of disk fluctuations
Kevin Flaherty, James Muzerolle, Scott Wolk +6
Variability in the infrared emission from disks around pre-main sequence stars over the course of days to weeks appears to be common, but the physical cause of the changes in disk…