activity
20242026
collaborators

18 papers

astro-ph.GA2026

Resolving dense photodissociation regions: the structure of photochemical fronts in three-dimensional gas distributions

Brandt A. L. Gaches, Thomas G. Bisbas, Lothar Brendel +1

For decades, the Orion Bar has been the prototypical photodissociation region. Viewed nearly edge-on, it offers a unique window into the stratified chemical structure of the atomic…

astro-ph.GA2026

A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity

Gan Luo, Marco Padovani, Daniele Galli +5

The cosmic-ray ionization rate (CRIR) is one of the fundamental parameters influencing the chemical and dynamical evolution of molecular clouds. Although observations in recent yea…

astro-ph.GA2026

The Colors of Ices: Measuring ice column density through photometry

Adam Ginsburg, Savannah R. Gramze, Matthew L. N. Ashby +8

Ices imprint strong absorption features in the near- and mid-infrared, but until recently they have been studied almost exclusively with spectroscopy toward small samples of bright…

astro-ph.IM2026

RAYTHEIA: A high-performance ray-tracing algorithm for three-dimensional direction-dependent equations in astronomical simulations

Zhengping Zhu, Thomas G. Bisbas, Xuefei Tang +3

We present RAYTHEIA, a high-performance reverse ray-tracing algorithm designed to efficiently solve three-dimensional direction-dependent equations in astronomical simulations. The…

astro-ph.GA2026

Complex organic molecules and cosmic ray ionisation rate towards the massive protostar Cepheus A HW2

Emma W. Nielsen, Anna Punanova, Eva Wirström +5

Cosmic rays (CRs) are important drivers for molecular chemistry in star-forming regions, and laboratory experiments have shown that CRs can stimulate the release of complex organic…

astro-ph.GA2026

Mapping CO Ice in a Star-Forming Filament in the 3 kpc Arm with JWST

Savannah Gramze, Adam Ginsburg, Nazar Budaiev +14

CO gas emission is a fundamental tool for measuring column density, but in cold, dark clouds, much of the CO is locked away in ice. We present JWST results from observations of a s…