How do environmental processes quench cluster galaxies?

Event Start:
2024-01-22T16:00:00
Event End:
2024-01-22T17:00:00
Event Information:

Abstract:

The Virgo Environment Traced in CO Survey (VERTICO) is an Atacama Large Millimeter/submillimeter Array Large Program that has mapped the distribution and kinematics of star-forming molecular gas across 51 Virgo Cluster satellite galaxies on sub-kpc scales. 

Event Location:
HENN 318
Speaker:
Dr. Toby Brown, Plaskett Fellow at the Herzberg Astronomy & Astrophysics Research Centre
Related Upcoming Events:
Add to Calendar Event Start: 2024-01-22T16:00:00 Event End: 2024-01-22T17:00:00 How do environmental processes quench cluster galaxies? Event Information: Abstract: The Virgo Environment Traced in CO Survey (VERTICO) is an Atacama Large Millimeter/submillimeter Array Large Program that has mapped the distribution and kinematics of star-forming molecular gas across 51 Virgo Cluster satellite galaxies on sub-kpc scales.  Event Location: HENN 318

Source URL: https://phas.ubc.ca/how-do-environmental-processes-quench-cluster-galaxies