collaborators

6 papers

astro-ph.GA2026

Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration

Shaunak Modak, Chris Hamilton, Eve C. Ostriker +1

Interstellar medium (ISM) structures gravitationally perturb stellar orbits in galactic disks, driving orbital heating and migration. However, studies of these transport processes…

astro-ph.GA2026

Characterizing Density and Gravitational Potential Fluctuations of the Interstellar Medium

Shaunak Modak, Eve C. Ostriker, Chris Hamilton +1

Substructure in the interstellar medium (ISM) is crucial for establishing the correlation between star formation and feedback and has the capacity to significantly perturb stellar…

astro-ph.GA2025

Galactokinetics

Chris Hamilton, Shaunak Modak, Scott Tremaine

Galactic disks lie at the heart of many of the most pressing astrophysical puzzles. There are sophisticated kinetic theories that describe some aspects of galaxy disk dynamics, but…

astro-ph.GA2025

Dynamical evolution of stellar binaries in galactic centers

Mark Dodici, Scott Tremaine, Yanqin Wu

Stellar binaries in galactic centers are relevant to several observable phenomena, including hypervelocity stars, X-ray binaries, and mergers of stars and compact objects; however,…

astro-ph.GA2025

Galactic echoes

Rimpei Chiba, Jupiter Ding, Chris Hamilton +2

Gaia has revealed a variety of substructures in the phase space of stars in the Solar neighborhood, including the vertical `Snail' in space. Such substructures are often…

astro-ph.GA2025

Galactokinetics II: Spiral structure

Chris Hamilton, Shaunak Modak, Scott Tremaine

We present a unified theory of linear spiral structure in stellar disks. We begin by identifying the characteristic scales involved in the spiral structure problem and listing some…