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Kavli Institute for Cosmology, Cambridge



Galaxy evolution
Physical processes quenching star formation.
- AGN radio-mode feedback.
- Gas content of green valley galaxies.


Key publications: 

What drives galaxy quenching? Resolving molecular gas and star formation in the green valley  (arXiv:2007.02976)

Detecting the halo heating from AGN feedback with ALMA (arXiv:1910.02088)

Teaching and Supervisions


2017-2020: Part 1A Mathematics for Natural Sciences 

 Sim  Brownson

Contact Details

Email address: 
Room K31
Kavli Institute for Cosmology, Cambridge
Institute of Astronomy
University of Cambridge
Madingley Road Cambridge CB3 0HA
United Kingdom
(01223) 337210


Person keywords: 
Galaxy formation and evolution

KICC Annual Report 2019

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