September 5 - September 9
Epoch of Galaxy Quenching 2022
at the Kavli Institute for Cosmology, Cambridge
A hybrid (online & on-site) meeting focusing on one of the most important problems in modern extra-galactic astronomy:
why do galaxies stop forming stars?
why do galaxies stop forming stars?
Key Scientific Questions
Chemical
Composition
Composition
How do the chemical compositions of star forming and quenched galaxies compare? What can we learn about the quenching process from measurements of metallicity in gas and stellar populations (e.g. outflows vs. strangulation)? Do contemporary models accurately reproduce the changes in metallicity of galaxies over the epoch of quenching?
Structure
& Kinematics
& Kinematics
What is the origin of the close connection between galactic star formation and structure/ kinematics/ morphology? How does galactic structure evolve from z ~ 2 to the present? Which processes engender the transition from discs to spheroids (e.g. major and minor mergers vs. violent disk instabilities)? How does this structural evolution impact star formation?
Star Formation
& Gas Content
& Gas Content
What is the origin of the star-forming main sequence (SFR -M* relation)? How does the main sequence evolve from cosmic noon to the present? What physical processes set the Kennicutt-Schmidt relation between gas surface density and the surface density of star formation rate? How does the gas content of galaxies impact star formation? How does star formation efficiency (and its inverse: depletion time) vary within and between galaxies? What can we learn about quenching from observations and simulations of gas in the IGM, CGM and ISM?
The Role
of Feedback
of Feedback
Is AGN feedback needed to quench massive galaxies? If so, by which specific mechanism(s) does it operate (e.g. heating vs. outflows)? What observational evidence exists for each scenario? Is supernova feedback responsible for regulating star formation in low mass galaxies? Are other feedback mechanisms important for galaxy quenching (e.g. cosmic rays, magnetic fields)? How do different feedback processes work together in simulations of galaxy evolution? What physical processes set the peak of the halo mass – stellar mass relation?
The Role
of Environment
of Environment
How does environment impact the star formation and quenching of central and satellite galaxies? What is the role of the dark matter halo in quenching? By what physical mechanisms do dense cluster environments quench satellite galaxies? Is galactic conformity real? If so, what is the mechanism by which quenching is ‘contagious’?
SOC
Debora Sijacki
(KICC, Co-chair)
Francesco D'Eugenio
(KICC, Co-chair)
Asa Bluck
(Florida International University)
Michele Cappellari
(University of Oxford)
Alice Concas
(ESO, Garching)
Emma
Curtis-Lake
(University of Hertfordshire)
Stephen Eales
(Cardiff University)
Sara Ellison
(University of Victoria)
Natascha
Förster-Schreiber
(MPE, Munich)
Julie Hlavacek-Larrondo
(Université de Montréal)
Roberto Maiolino
(KICC)
Annalisa Pillepich
(MPIA, Heidelberg)
Yingjie Peng
(KIAA, Beijing)
Joop Schaye
(Leiden Observatory)
Jan Scholtz
(KICC)
LOC
William Baker
Asa Bluck
Steven Brereton
(admin)
(admin)
Emma
Curtis-Lake
Curtis-Lake
Tobias Looser
Gabriel Maheson
Roberto Maiolino
Joanna Piotrowska
Lester Sandles
CONTACT US
quench2022@kicc.cam.ac.uk