activity
20242026
most citedThe 3D Structure and Kinematics of the Local Disk-Halo Interface: Intermediate-velocity Clouds are the Minority of High-altitude Clouds in the Solar Neighborhood

1 citations · 1 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

The Multi-phase HI of the Milky Way and Nearby Galaxies

Marc-Antoine Miville-Deschênes, J. R. Dawson, Narendra Nath Patra +30

Atomic hydrogen (HI) is the dominant baryonic component of the interstellar medium (ISM) in Milky Way-like galaxies and the reservoir from which molecular clouds and stars ultimate…

astro-ph.GA20261 cited

The 3D Structure and Kinematics of the Local Disk-Halo Interface: Intermediate-velocity Clouds are the Minority of High-altitude Clouds in the Solar Neighborhood

Theo J. O'Neill, Andrew K. Saydjari, Catherine Zucker +4

Studies of the Milky Way's disk-halo interface have historically identified inflowing and outflowing gas incompatible with disk rotation on the basis of radial velocity, leading to…

astro-ph.GA2026

Filamentary Hierarchies and Superbubbles II: Impact of superbubbles and galactic dynamics on filament formation and fragmentation

Rachel Pillsworth, Ralph E. Pudritz, Eric W. Koch +1

Large scale phenomena in spiral galaxies such as shear, supernovae, and magnetic fields all contribute to the formation and subsequent evolution of filamentary structure and star f…

astro-ph.GA2025

A 3D Model of the Local Bubble's Magnetic Field: Insights from Dust and Starlight Polarization

Theo J. O'Neill, Alyssa A. Goodman, Juan D. Soler +2

Clustered stellar feedback creates expanding voids in the magnetized interstellar medium known as superbubbles. Although theory suggests that superbubble expansion is influenced by…

astro-ph.GA2025

Origin of the IRAS Vela Shell: New Insights from 3D Dust Mapping

Bore Annie Gao, Catherine Zucker, Tirupati Kumara Sridharan +15

The IRAS Vela Shell (IVS) is a structure of enhanced FIR emission located towards the Gum Nebula, a prominent region of emission in the local Milky Way shaped by various…

astro-ph.GA2024

The Local Bubble is a Local Chimney: A New Model from 3D Dust Mapping

Theo J. O'Neill, Catherine Zucker, Alyssa A. Goodman +1

Leveraging a high-resolution 3D dust map of the solar neighborhood from Edenhofer et al. (2024), we derive a new 3D model for the dust-traced surface of the Local Bubble, the super…