activity
20242026
collaborators

11 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.GA2026

A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XX. Star formation in the tidal tail of NGC 4254

A. Boselli, A. Lupi, P. Serra +26

ALMA 12CO(1-0) observations of 42 star-forming regions located outside the disc of the Virgo Cluster galaxy NGC4254 within an HI gas tail produced during the galaxy's interaction w…

astro-ph.GA2026

Turning JWST/MIRI backgrounds into a survey of diffuse molecular hydrogen

E. Nigou, B. Godard, P. Guillard +3

Context. A statistically significant sampling of H2 rotational excitation in the diffuse interstellar medium (ISM) is essential to identifying its excitation mechanisms and assessi…

astro-ph.GA2026

Are supernovae driving turbulence in the solar neighborhood?

Georges Abboudeh, Patrick Hennebelle, Juan D. Soler +9

Turbulence plays an important role in shaping the interstellar medium, and strongly influences star formation. We aim to identify the physical processes capable of sustaining HI tu…

astro-ph.GA2026

JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium

G. Vigoureux, N. Flagey, F. Boulanger +14

Interstellar medium studies rely on magnetohydrodynamic (MHD) turbulence as a framework for interpretation. In this context, the statistical characterization of interstellar observ…

astro-ph.GA2026

The contribution of neutral gas to Faraday tomographic data at low frequencies. A first extensive comparison between real and synthetic data

Jack Berat, Marc-Antoine Miville-Deschênes, Andrea Bracco +2

LOFAR observations of diffuse interstellar polarization at meter wavelengths reveal intricate polarized intensity structures with an unexpected correlation with neutral HI filament…