activity
20182020
most citedNew Constraints From Dust Lines On The Surface Densities Of Protoplanetary Disks

62 citations · 75 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202013 cited

A collage of small planets from the Lick Carnegie Exoplanet Survey : Exploring the super-Earth and sub-Neptune mass regime

Jennifer A. Burt, Fabo Feng, Bradford Holden +12

Analysis of new precision radial velocity (RV) measurements from the Lick Automated Planet Finder (APF) and Keck HIRES have yielded the discovery of three new exoplanet candidates…

astro-ph.EP2020

How Consumption and Repulsion Set Planetary Gap Depths and the Final Masses of Gas Giants

Mickey Rosenthal, Eugene Chiang, Sivan Ginzburg +1

Planets open gaps in discs. Gap opening is typically modeled by considering the planetary Lindblad torque which repels disc gas away from the planet's orbit. But gaps also clear be…

astro-ph.EP2019

Measuring the Orbital Parameters of Radial Velocity Systems in Mean Motion Resonance---a Case Study of HD 200964

M. M. Rosenthal, W. Jacobson-Galan, B. Nelson +8

The presence of mean motion resonances (MMRs) complicates analysis and fitting of planetary systems observed through the radial velocity (RV) technique. MMR can allow planets to re…

astro-ph.EP2019

How Flow Isolation May Set the Mass Scale for Super-Earth Planets

M. M. Rosenthal, R. A. Murray-Clay

Much recent work on planet formation has focused on the growth of planets by accretion of grains whose aerodynamic properties make them marginally coupled to the nebular gas, a the…

astro-ph.EP201962 cited

New Constraints From Dust Lines On The Surface Densities Of Protoplanetary Disks

Diana Powell, Ruth Murray-Clay, Laura M. Pérez +2

We present new determinations of disk surface density, independent of an assumed dust opacity, for a sample of 7 bright, diverse protoplanetary disks using measurements of disk dus…

astro-ph.EP2018

Restrictions on the Growth of Gas Giant Cores via Pebble Accretion

M. M. Rosenthal, R. A. Murray-Clay

We apply an order-of-magnitude model of gas-assisted growth, known as pebble accretion, in a turbulent medium to suggest a reason why some systems form wide orbital separation gas…