Name: Interstellar Institute 7
Start: 2025-07-07T09:00:00+02:00
End: 2025-07-25T17:00:00+02:00
Location: Institut Pascal

lundi 7 juillet 2025 ¶

09:30 Lightning
Lightning
09:30 - 10:00

10:00 Super-Extended Multi-Parsec Dust Emission, and Strange Dust Properties, Revealed Around AGB Stars
Super-Extended Multi-Parsec Dust Emission, and Strange Dust Properties, Revealed Around AGB Stars
10:00 - 10:25

10:25 Statistical Analysis of PAHs as a Tracer of Anomalous Microwave Emission
Statistical Analysis of PAHs as a Tracer of Anomalous Microwave Emission
10:25 - 10:50

10:50 Constraints on rotational disruption of dust grains based on the survival of the zodiacal cloud
Constraints on rotational disruption of dust grains based on the survival of the zodiacal cloud
10:50 - 11:15

11:15 Dusty-PRISM: Predicting the evolution of dust and PAHs across cosmic time with cosmic rays, magnetic fields and radiation-hydrodynamics simulations of galaxy formation
Dusty-PRISM: Predicting the evolution of dust and PAHs across cosmic time with cosmic rays, magnetic fields and radiation-hydrodynamics simulations of galaxy formation
11:15 - 11:40
mardi 8 juillet 2025 ¶

10:00 The Impact of Chemistry on Multiphase ISM Simulations
The Impact of Chemistry on Multiphase ISM Simulations
10:00 - 10:25

10:25 Impact of the Supernova remnants in the interstellar matter of our galaxy
Impact of the Supernova remnants in the interstellar matter of our galaxy
10:25 - 10:50

10:50 JWST observations of the magnetized ISM in the Pleiades
JWST observations of the magnetized ISM in the Pleiades
10:50 - 11:15

11:15 Local Map of Interstellar UV Field
Local Map of Interstellar UV Field
11:15 - 11:40

17:00 Happy hour
Happy hour
17:00 - 18:00
mercredi 9 juillet 2025 ¶

10:00 Deep 21cm observations of nearby galaxies
Deep 21cm observations of nearby galaxies
10:00 - 10:25

10:25 Spatial Structure of Cold HI Gas Properties in the Milky Way with GASKAP
Spatial Structure of Cold HI Gas Properties in the Milky Way with GASKAP
10:25 - 10:50

10:50 Reconstructing the ISM with Bayesian Spectral Models
Reconstructing the ISM with Bayesian Spectral Models
10:50 - 11:15

11:15 A consistent view of the dusty, polarized Galaxy: from magnetically aligned HI gas to polarization power spectra
A consistent view of the dusty, polarized Galaxy: from magnetically aligned HI gas to polarization power spectra
11:15 - 11:40

14:00 Bayesian Spectral Models
Bayesian Spectral Models
14:00 - 14:25
jeudi 10 juillet 2025 ¶

10:00 Conditions for molecular cloud formation: an atomic and molecular perspective
Conditions for molecular cloud formation: an atomic and molecular perspective
10:00 - 10:25

10:25 Unveiling the CO-dark gas properties of our Galaxy
Unveiling the CO-dark gas properties of our Galaxy
10:25 - 10:50

10:50 Mapping 3D Distributions of HI and CO in the Milky Way
Mapping 3D Distributions of HI and CO in the Milky Way
10:50 - 11:15

11:15 Scattering Transforms in astrophysics, application to components separation
Scattering Transforms in astrophysics, application to components separation
11:15 - 11:40

14:00 Pulsar timing : DM, RM and HI absorption
Pulsar timing : DM, RM and HI absorption
14:00 - 15:00

19:00 Dinner at Le Gramophone
Dinner at Le Gramophone
19:00 - 21:00
vendredi 11 juillet 2025 ¶

10:00 Magnetic fields in the multiphase ISM of the Milky Way
Magnetic fields in the multiphase ISM of the Milky Way
10:00 - 10:25

10:25 Angular momentum in molecular clouds and filaments: Transfer mechanisms, 3D dynamics, and relative orientation with respect to outflows
Angular momentum in molecular clouds and filaments: Transfer mechanisms, 3D dynamics, and relative orientation with respect to outflows
10:25 - 10:50

10:50 Ambipolar diffusion and the mass-to-flux ratio in turbulent collapsing clouds
Ambipolar diffusion and the mass-to-flux ratio in turbulent collapsing clouds
10:50 - 11:15

11:15 Gravity at work: energy budget in simulated molecular clouds
Gravity at work: energy budget in simulated molecular clouds
11:15 - 11:40

15:00

15:00 - 15:30
samedi 12 juillet 2025 ¶
dimanche 13 juillet 2025 ¶

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