12:25 PM
|
--- lunch ---
|
1:25 PM
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Posters
(until 1:35 PM)
(Eridanus Auditorium)
|
1:25 PM
|
Evolution of galactic magnetic fields in HI defined interaction stages.
-
Ancor Damas
(Instituto de Astrofísica de Andalucía (iaa-CSIC))
(Eridanus Auditorium)
|
1:26 PM
|
Spin alignment in CHILES
-
Julia Gross
(Columbia University)
(Eridanus Auditorium)
|
1:27 PM
|
A new perspective on group finding
-
Zackary Hutchens
(University of North Carolina at Chapel Hill)
(Eridanus Auditorium)
|
1:28 PM
|
The impact of local photoionization sources on simulated galaxies: evolution of HI disks
-
Aura Obreja
(University Observatory Munich)
(Eridanus Auditorium)
|
1:29 PM
|
Properties of AU-scale structure from 21-SPONGE observations
-
Daniel Rybarczyk
(University of Wisconsin-Madison)
(Eridanus Auditorium)
|
1:30 PM
|
Predictions of detections of high mass galaxies in CHILES
-
Monica Sanchez Barrantes
(UNM, NRAO)
(Eridanus Auditorium)
|
1:35 PM
|
Theory (and related observations) [chair: Romeel Dave]
(until 3:05 PM)
(Eridanus Auditorium)
|
1:35 PM
|
From the ISM to the gas around galaxies: perspective from numerical simulations
-
Dusan Keres
(UC San Diego)
(Eridanus Auditorium)
|
2:05 PM
|
Galaxy formation with feedback from individual stars
-
Thorsten Naab
(Max-Planck-Institute for Astrophysics)
(Eridanus Auditorium)
|
2:25 PM
|
The effects of local stellar radiation on non-equilibrium ISM chemistry and ISM line diagnostics
-
Alex Richings
(Durham University)
(Eridanus Auditorium)
|
2:45 PM
|
The evolution of the interstellar medium in merging galaxies
-
Jorge Moreno
(Pomona College)
(Eridanus Auditorium)
|
3:05 PM
|
--- coffee ---
|
3:35 PM
|
Theory (and related observations) [chair: Romeel Dave]
(until 4:55 PM)
(Eridanus Auditorium)
|
3:35 PM
|
Prevalence of neutral gas in centres of merging galaxies
-
Rajeshwari Dutta
(European Southern Observatory, Garching)
(Eridanus Auditorium)
|
3:55 PM
|
The startling dynamics of HI-rich ultra-diffuse galaxies
-
Pavel Mancera Piña
(Kapteyn Astronomical Institute & ASTRON)
(Eridanus Auditorium)
|
4:15 PM
|
How can HI dynamics be used to probe the connection between galaxies and their dark matter halos over cosmic time?
-
Federico Lelli
(European Southern Observatory)
(Eridanus Auditorium)
|
4:35 PM
|
How HI populates haloes: simulations vs. observations
-
Garima Chauhan
(ICRAR/UWA)
(Eridanus Auditorium)
|
4:55 PM
|
discussion
(Eridanus Auditorium)
|