July 28, 2025 to August 1, 2025
Perimeter Institute for Theoretical Physics
America/Toronto timezone

Investigating Galaxy Ecosystems with Multi-wavelength Observations of Gas and Dust

Jul 31, 2025, 11:30 a.m.
10m
PI/1-100 - Theatre (Perimeter Institute for Theoretical Physics)

PI/1-100 - Theatre

Perimeter Institute for Theoretical Physics

190
Contributed Talk

Speaker

Prof. Varsha Kulkarni (University of South Carolina)

Description

We report results from observations of the CGM ionized, atomic, molecular, and condensed phases using a combination of integral field spectroscopy (MaNGA, VLT MUSE, JWST MRS), and imaging and spectroscopy from HST, VLT, Magellan. In a study of the warm and cool CGM of galaxies mapped with IFS, and a comparison of the kinematics, ionization, and metallicity of this gas with the ionized gas in star-forming regions in the galaxies, we find consistency with a co-rotation of the cool CGM with galaxy disks and hints of changes in gas ionization, potentially due to the stronger intergalactic radiation field at larger galactocentric distance. Our spatially resolved maps of gas metallicity and ionization around galaxies provide constraints on models of the metal distribution around galaxies. Our results are also consistent with higher metallicity and higher ionization parameter for gas at higher elevation angles, as expected for outflows. Our JWST studies of the composition, structure, and extinction properties of the dust grains in both the diffuse and dense ISM/CGM of galaxies at 0<z<1.5 indicate that dust grains in distant galaxies differ in physical and chemical properties from grains in local galaxies. Finally, our study of the ISM/CGM at 4<z<6 shows that high-redshift galaxies show a wide diversity of chemical enrichment histories, including some cases of highly accelerated chemical evolution.

We gratefully acknowledge support from NASA/STScI grants for HST GO-15939, GO-16242, GO-17121, JWST GO-2155, GO-5491, and from NASA grant 80NSSC20K0887.

Primary Theme Hot gas to cold gas
Secondary Theme Diffuse to dense structures
Presenter's Name Varsha P. Kulkarni
Presenter's Email Address [email protected]
Keywords warm/cool CGM, dust, metal distribution, kinematics, co-rotation, ionization, IFS, evolution
Recording Permission YES
Virtual Audience Permission YES
Photography Permission YES
If your talk is not accepted for a contributed talk, would you be interested in presenting a fireslide/lightning talk? No
If your fireslide/lighting talk is not accepted, would you be interested in presenting a poster? No

Author

Prof. Varsha Kulkarni (University of South Carolina)

Co-authors

Dr Viacheslav Klimenko (University of South Carolina) Mr Arjun Karki (University of South Carolina) Mr Jianghao Huyan (University of South Carolina) Dr Celine Peroux (ESO) Dr Monique Aller (Georgia Southern University) Dr Ramona Augustin (AIP, Potsdam) Dr Simon Weng (Laboratoire d'Astrophysique de Marseille) Prof. David Wake (University of North Carolina, Asheville) Prof. Matthew Bershady (University of Wisconsin, Madison) Prof. Britt Lundgren (University of North Carolina, Asheville) Prof. Sebastian Lopez (Universidad de Chile) Prof. Nicolas Tejos (Pontificia Universidad Católica de Valparaíso)

Presentation materials

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External references