Lightning

Super-Extended Multi-Parsec Dust Emission, and Strange Dust Properties, Revealed Around AGB Stars

Statistical Analysis of PAHs as a Tracer of Anomalous Microwave Emission

Constraints on rotational disruption of dust grains based on the survival of the zodiacal cloud

Dusty-PRISM: Predicting the evolution of dust and PAHs across cosmic time with cosmic rays, magnetic fields and radiation-hydrodynamics simulations of galaxy formation

The Impact of Chemistry on Multiphase ISM Simulations

Impact of the Supernova remnants in the interstellar matter of our galaxy

JWST observations of the magnetized ISM in the Pleiades

Local Map of Interstellar UV Field

Happy hour

Deep 21cm observations of nearby galaxies

Spatial Structure of Cold HI Gas Properties in the Milky Way with GASKAP

Reconstructing the ISM with Bayesian Spectral Models

A consistent view of the dusty, polarized Galaxy: from magnetically aligned HI gas to polarization power spectra

Bayesian Spectral Models

Conditions for molecular cloud formation: an atomic and molecular perspective

Unveiling the CO-dark gas properties of our Galaxy

Mapping 3D Distributions of HI and CO in the Milky Way

Scattering Transforms in astrophysics, application to components separation

Pulsar timing : DM, RM and HI absorption

Dinner at Le Gramophone

Magnetic fields in the multiphase ISM of the Milky Way

Angular momentum in molecular clouds and filaments: Transfer mechanisms, 3D dynamics, and relative orientation with respect to outflows

Ambipolar diffusion and the mass-to-flux ratio in turbulent collapsing clouds

Gravity at work: energy budget in simulated molecular clouds

High-Altitude Clouds in the Solar Neighborhood: Connecting 3D Dust Maps and HI Gas Kinematics

Reconstructing the 3+1D Velocity Field of the Milky Way from Dust Absorption

Reconstructing the 3+1D Velocity Field of the Milky Way from Dust Absorption

Atomizing the "spiral structure" of the Milky Way Galaxy

Strong turbulence and magnetic coherent structures in galaxies

My White Whale: A Galactic-scale Parker Spiral?

My White Whale: A Galactic-scale Parker Spiral?

MilkyWay3D: A Data-Rich Online Environment for Exploring Our Galactic Neighborhood

GASKAP-HI Gaussian Decomposition Working group

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The Cold Gas of the Magellanic Cloud

HI Absorption with GASKAP-HI

Probabilistic Machine Learning Techniques for Mapping Neutral Hydrogen Gas Phases

An Aperture Synthesis Mosaic of the Small Magellanic Cloud with ASKAP - A non-linear optimization approach to joint deconvolution

Exploring Protostellar Jets in Star Cluster Formation with Torch

3D reconstruction of the interstellar magnetic field orientation

Galactic magnetic field tomography in the spiral arms using optical and near-infrared starlight polarization

Reconstructing the kinetic energy and momentum densities in the nearby interstellar medium (and Galactic scale numerical simulations)

Dinner at Le Gramophone

Multiscale Models of Star Cluster Formation and Early Dynamics

Environmental Quenching through the lens of Small-scale ISM Physics

Hot CGM: the hidden treasure trove of galaxies

Zooming-in on the turbulence cascade, from galactic scales to prestellar cores

Revealing a nearby giant gas structure

The Closest Dark Molecular Cloud to the Solar System Revealed via H2 Fluorescence

ISRF-3D: A Code Suite for Three-dimensional Interstellar Radiation Field Modeling Using HEALPix Voxels

What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the ISM

LMC: A Case Study to Uncover its Magnetic Fields

Synthetic Faraday sky observed within a Local Bubble-like cavity

A 3D dust polarization map of the solar neighbourhood

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Diffuse filamentary emission from the Polarisation Sky Survey of the Universe's Magnetism (POSSUM)

Correlation between diffuse gas phases and Faraday tomographic data : a numerical point of view

A mass invariant in a compressible turbulent medium

Mapping the ISM at Parsec-Scales with Dust Extinction in the Magellanic Clouds

The first detection of cosmic-ray excited H2 in interstellar space

Cold Neutral Medium of Local Starburst IC10 As Revealed By Neutral Hydrogen Absorption

GMIMS update

Detecting Molecular Hydrogen (H2) Emission at Cosmic Dawn

Dinner at Le Gramophone

Diffuse Interstellar Bands and the interstellar reddening law

The dust extinction curve: beyond R(V)