collaborators

5 papers

astro-ph.EP2026

A Retrieval Framework for Observationally Constraining the Parameters of Circumplanetary Disks

Aster Taylor, Fred Adams

As they form, giant planets are surrounded by disks of gas and dust sourced from the background circumstellar disk. Although there have been few detections to date, upcoming instru…

astro-ph.EP2025

The Two-Dimensional Structure of Circumplanetary Disks and their Radiative Signatures

Aster G. Taylor, Fred C. Adams, Nuria Calvet

During their formative stages, giant planets are fed by infalling material sourced from the background circumstellar disk. Due to conservation of angular momentum, the incoming gas…

astro-ph.EP2025

Theoretical Mass Function for Secondaries Forming via Gravitational Instability in Circumstellar Disks

Fred C. Adams, Aster G. Taylor, Michael R. Meyer

This paper constructs a theoretical framework for calculating the distribution of masses for secondary bodies forming via gravitational instability in the outer regions of circumst…

astro-ph.EP2025

Determination of Jupiter's Primordial Physical State

Konstantin Batygin, Fred C. Adams

The formation and early evolution of Jupiter played a pivotal role in sculpting the large-scale architecture of the solar system, intertwining the narrative of Jovian early years w…

astro-ph.EP2025

General Analytic Solutions for Circumplanetary Disks during the Late Stages of Giant Planet Formation

Fred C. Adams, Konstantin Batygin

Forming giant planets are accompanied by circumplanetary disks, as indicated by considerations of angular momentum conservation, observations of candidate protoplanets, and the sat…