activity
20172025
most citedSEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

128 citations · 634 across the 19 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2025

Characterizing the interplay between Galactic star formation and ionization feedback with PRIMA

Annie Zavagno, Delphine Russeil, Paolo Suin +13

Recent results from the James Webb Space Telescope show that nearby spiral galaxies are dominated by the presence of H I and H II bubbles that strongly shape their surrounding medi…

astro-ph.GA2025

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…

astro-ph.GA2025

Structure and Fragmentation Scale of a Massive Star-Forming Filament in NGC6334: High-Resolution Mid-Infrared Absorption Imaging with JWST

Philippe André, Michael Mattern, Doris Arzoumanian +4

Dense filaments are believed to be representative of the initial conditions of star formation in molecular clouds. We have used the MIRI instrument on JWST to image the massive fil…

astro-ph.GA2024★ 10 cited

Understanding the Star Formation Efficiency in Dense Gas: Initial Results from the CAFFEINE Survey with ArTéMiS

M. Mattern, Ph. André, A. Zavagno +9

Despite recent progress, the question of what regulates the star formation efficiency in galaxies remains one of the most debated problems in astrophysics. According to the dominan…

astro-ph.GA2022★ 3 cited

ArTéMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps

Oskari Miettinen, Michael Mattern, Philippe André

We imaged the infrared dark clouds (IRDCs) G1.75-0.08 and G11.36+0.80 at 350 m and 450 m using the ArTéMiS bolometer. These data were used in conjunction with our previous 87…

astro-ph.GA2022★ 9 cited

The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties

K. R. Neralwar, D. Colombo, A. Duarte-Cabral +21

The Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium (SEDIGISM) survey has produced high (spatial and spectral) resolution CO (2-1) maps of the…