collaborators

8 papers

astro-ph.HE2026

A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density

Hanieh Zandinejad, Jakob Roth, Vo Hong Minh Phan +7

Cosmic rays (CRs) are a ubiquitous non-thermal component of the interstellar medium (ISM). A data-driven three-dimensional (3D) map of their distribution is essential for understan…

astro-ph.GA2025

The superclouds of the local Milky Way

Lilly A. Kormann, João Alves, Michelangelo Pantaleoni González +3

Recent 3D dust maps of the local Milky Way are revolutionizing our understanding of the Sun's Galactic neighborhood, providing much needed insight into the large-scale organization…

astro-ph.GA2025

Spatially Coherent 3D Distributions of HI and CO in the Milky Way

Laurin Söding, Gordian Edenhofer, Torsten A. Enßlin +6

The spatial distribution of the gaseous components of the Milky Way is of great importance for a number of different fields, for example, Galactic structure, star formation, and co…

astro-ph.HE2025

The influence of the 3D Galactic gas structure on cosmic-ray transport and -ray emission

Andrés Ramírez, Gordian Edenhofer, Torsten A. Enßlin +6

Cosmic rays (CRs) play a major role in the dynamics of the interstellar medium (ISM). Their interactions and transport ionize, heat, and push the ISM thereby coupling different reg…

astro-ph.GA2025

A Deep, High-Angular Resolution 3D Dust Map of the Southern Galactic Plane

Catherine Zucker, Andrew K. Saydjari, Joshua S. Speagle +8

We present a deep, high-angular resolution 3D dust map of the southern Galactic plane over and built on photometry from the DECaPS2 su…

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…