Description |
Understanding the connection of local galaxies to their circumgalactic medium (CGM) is crucial for establishing a robust comparison sample for studies of the interactions of higher-redshift galaxies with their surroundings. I will report results from our recent imaging and spectroscopic studies aimed at understanding how CGM properties and stellar properties correlate. In a study of star-forming galaxies at redshifts 0.02 |
Organised by | DAA |