Program
Session Plan
Each 90 minute session will begin with one invited talk to appropriately set the scene (20+5 minutes) followed by five contributed and invited talks (10+3 minutes). The contributed talks will be selected to present exciting results that highlight new avenues of research and/or synergies between different wavebands or theory and observation.
- Assessing cold ISM structure in galaxies across scales and the processes shaping it through spatially resolved observations (2 sessions).
- Relationship between cold gas and dust (1 session).
- Impact of star formation and active galactic nuclei on their surrounding cold ISM and how this is best probed by infrared and radio instruments (2 sessions).
- Radio and infrared probes of astrochemistry and ISM physical properties (1 session).
Accepted talks (alphabetical last name order by session)
Assessing cold ISM structure in galaxies across
scales and the processes shaping it through spatially resolved observations |
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# |
First Name |
Last Name |
Title |
2135 |
Barbara |
Catinella |
Linking atomic and molecular gas
stripping with quenching in satellite galaxies at different infall stages |
2233 |
Cosima |
Eibensteiner |
PHANGS-MeerKAT and MHONGOOSE HI
observations of nearby spiral galaxies: physical drivers of the molecular gas
fraction, Rmol |
2337 |
Petro |
Janse van Rensburg |
Studying gas flows in nearby
SUNBIRD starburst galaxies and LIRGs |
1456 |
Ryan |
Keenan |
Molecular Gas Conditions and CO
Line Excitation in Nearby Galaxies with AMISS |
951 |
Shinjeong |
Kim |
Cold gas formation within an HI
shell in the Magellanic Bridge from GASKAP-HI
observations |
2494 |
Adam |
Leroy |
Cold ISM Structure and Feedback on
Multiple Scales in Nearby Galaxies |
1865 |
Nora |
Linzer |
Ultraviolet Radiation Fields and
Gas/Dust Emission in Star-Forming Disk Galaxies: Numerical Simulations with
TIGRESS-NCR |
2029 |
Naomi |
McClure-Griffiths |
A GASKAP-HI View of Atomic Hydrogen
in the Milky Way and Magellanic Clouds |
1037 |
Rowan |
Smith |
The origin of cold ISM structure:
insights from the dialogue between spatially resolved observations and high resolution simulations |
1003 |
Juan |
Soler |
Connecting molecular clouds to
their Galactic environment using neutral atomic hydrogen (HI) and 3D dust
maps |
957 |
Yu-Hsuan (Eltha) |
Teng |
Star Formation Efficiency in Nearby
Galaxies Revealed with a New CO-to-H2 Conversion Factor Prescription |
1703 |
Nikki |
Zabel |
Resolved studies of the atomic and
molecular gas in cluster galaxies in the era of ALMA, MeerKAT, and the SKA |
Relationship between cold gas and dust |
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# |
First Name |
Last Name |
Title |
2884 |
Chloe |
Bosomworth |
Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda
Galaxy |
2605 |
Alice |
Concas |
Molecular gas and dust extinction
relation revealed by ALMAQUEST |
2154 |
Debosmita |
Pathak |
The Distribution and Impact of
Mid-Infrared Emission in Nearby Galaxies |
1521 |
Michael |
Romano |
New evidence for outflow-induced
gas and dust enrichment in the surroundings of dwarf galaxies |
2587 |
Karin |
Sandstrom |
The Relationship Between Cold Dust
and Gas |
2587 |
Farhard |
Yusef-Zadeh |
Highlights of MeerKAT Survey of the
Galactic Center Region |
Impact of star formation and active galactic nuclei
on their surrounding cold ISM and how this is best probed by infrared and
radio instruments |
|||
# |
First Name |
Last Name |
Title |
1607 |
Henco |
Arlow |
The gas content of Luminous Compact
Blue Galaxies in the COSMOS field |
2357 |
Anelise |
Audibert |
Feedback from low-power radio jets
on the gas reservoirs of quasars |
1070 |
Loreto |
Barcos-Muñoz |
Star Formation and Feedback in
Local Luminous and Ultra Luminous Infrared Galaxies |
474 |
Edvige |
Corbelli |
Star formation drivers in the local
universe |
968 |
Deanne |
Fisher |
How galaxies regulate their growth |
1709 |
Filippo Marcello |
Maccagni |
Multi-phase and multi-wavelength:
the feeding and feedback AGN cycle revealed by sensitive observations of the
ISM |
2215 |
Thato |
Manamela |
OH megamasers at high redshifts |
1060 |
Tom |
Oosterloo |
Closing the feedback-feeding loop
of the radio galaxy 3C 84 |
3136 |
Ezequiel |
Treister |
Properties of the Molecular and
Atomic Gas in AGN in Mergers from ALMA and VLT/MUSE Observations |
2747 |
Stefanie |
Walch |
The impact of feedback on the cold
interstellar medium |
2374 |
Fabian |
Walter |
ALMA few-100pc imaging of z~7
quasar host galaxies |
1421 |
Maria Vittoria |
Zanchettin |
AGN feedback and ISM properties in
the nearby Universe |
Radio and infrared probes of astrochemistry and ISM
physical properties |
|||
# |
First Name |
Last Name |
Title |
2149 |
Ivana |
Bešlić |
When
astronomy meets data science: Exploring mm molecular lines emission across
Orion B |
1635 |
Bop |
Cheikh |
Exploring
Kinematics in the Early Phases of Star Formation through Deuterium
Fractionation |
2998 |
Kimberly |
Emig |
Cold
'dark' gas in Cygnus X: The first large-scale mapping of low-frequency carbon
recombination lines |
2025 |
Nanase |
Harada |
Astrochemical
diagnostics in various scales |
2717 |
Bo |
Peng |
Bridging
the gap between far-infrared fine structure lines and optical strong lines in
studying interstellar medium and star formation |
2805 |
Mavis |
Seidu |
MeerKAT's detection of low surface brightness HII regions associated with
highly variable 6.7 GHz methanol masers |
Invited
review |
Invited
short talk |