‹ Tuesday, September 26, 2023 › | |
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›8:30 (30min)
8:30 - 9:00 (30min)
Registration
Registration
9:00 - 10:15 (1h15)
Dust properties
RunAn
Karl Gordon
› There and back again — Dust evolution between diffuse and dense environments — It's complicated
- Anthony Jones, Institut d'Astrophysique Spatiale (IAS Orsay)
09:00-09:30 (30min)
› Dust Evolution across the Orion Bar: new insights from the JWST
- Meriem El Yajouri, Institut d'Astrophysique Spatiale (IAS) [France]
09:30-09:45 (15min)
› PASIPHAE Survey: Large optical polarimetric sky survey for dust cloud & magnetic field tomography
- Siddharth Maharana, South African Astronomical Observatory
09:45-10:00 (15min)
› Small amounts of iron(II) sulphides can significantly affect the SEDs of circumstellar disks
- Christian Kranhold, Astrophysical Institute and University Observatory, Friedrich-Schiller-University Jena
10:00-10:15 (15min)
›10:15 (45min)
10:15 - 11:00 (45min)
Coffee break
11:00 - 12:00 (1h)
Dust properties
RunAn
Gunnar Nyman
› Assessing the astronomical relevance of interstellar nanosilicate dust grains from IR spectra: theory, experiment and observation
- Stefan Bromley, Institució Catalana de Recerca i Estudis Avançats [Barcelona], Universitat de Barcelona
11:00-11:30 (30min)
› Exploring the dust properties in the nearby diffuse interstellar medium with JWST
- Sascha Zeegers, Sascha Zeegers, ESA - ESTEC (Netherlands)
11:30-11:45 (15min)
› Studying dust grain properties and growth by combining extinction and depletion measurements in the Milky Way
- Marjorie Decleir, Space Telescope Science Institute
11:45-12:00 (15min)
›12:00 (1h30)
12:00 - 13:30 (1h30)
Lunch
13:30 - 14:30 (1h)
Dust properties
RunAn
Dimitra Rigopoulou
› What do dust grains look like at the onset of the star and disk formation sequence ?
- Anaëlle Maury, Unité Mixte CEA/CNRS AIM, Université Paris Saclay
13:30-14:00 (30min)
› Modelling the cold dust in nearby spiral galaxies with radiative transfer
- Angelos Nersesian, Ghent University
14:00-14:15 (15min)
› The X-ray view of dust in the Milky Way
- Elisa Costantini, SRON Netherlands Institute for Space Research, Astronomical Institute Anton Pannekoek
14:15-14:30 (15min)
›14:30 (45min)
14:30 - 15:15 (45min)
Coffee break
15:15 - 16:45 (1h30)
Dust properties
RunAn
Wouter Vlemmings
› Dust Properties from the Lab applied to young disks: 3D-printing and a Microwave Analogy Experiment
- Francois MENARD, IPAG- Institut de Planetologie et d'Astrophysique de Grenoble
15:15-15:45 (30min)
› The influence of a clumpy outflow and companion star on the surface composition of AGB dust
- Marie Van de Sande, University of Leeds
15:45-16:00 (15min)
› The far-UV-extinction-to-H2 correlation and insights from IR emission in photodissociation regions
- Dries Van De Putte, Space Telescope Science Institute
16:00-16:15 (15min)
› The Si K Edge Gas and Dust Optical Depths Toward the Galactic Bulge
- Jun Yang, Massachusetts Institute of Technology
16:15-16:30 (15min)
› Investigating the Magnetic Fields under stellar feedback using dust polarization
- Ekta Sharma, National Astronomical Observatories of China
16:30-16:45 (15min)
16:45 - 17:00 (15min)
Poster flash session
RunAn
›17:00 (1h30)
17:00 - 18:30 (1h30)
Poster session and mingle
›19:00 (3h)
19:00 - 22:00 (3h)
Astronomy on Tap
Astronomy on Tap
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Session | Speech | Logistics | Break | Tour |