Thesis
The influence of morphology, AGN and environment on the quenching histories of galaxies
- Abstract:
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What drives the transition of galaxies from the disc dominated, star forming blue cloud to the elliptical dominated, quiescent red sequence? What role does the morphology, central supermassive black hole and galaxy environment play in this transition?
I have attempted to answer these questions by using Bayesian statistics to infer a simple star formation history (SFH) describing the time, tq, and exponential rate, τ, that quenching occurs in a galaxy. I use both...
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Authors
Contributors
+ Lintott, C
Department:
Physics
Role:
Supervisor
+ Davies, R
Department:
Physics
Role:
Examiner
+ Pimblett, K
Department:
University of Hull
Role:
Examiner
Funding
+ Science and Technology Facilities Council
More from this funder
Funding agency for:
Smethurst, R
Grant:
ST/K502236/1
Bibliographic Details
- Type of award:
- DPhil
- Level of award:
- Doctoral
- Awarding institution:
- University of Oxford
Item Description
- Language:
- English
- Keywords:
- Subjects:
- UUID:
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uuid:c7023345-ec69-42c3-907e-32c12a9ee115
- Deposit date:
- 2017-05-31
Related Items
Terms of use
- Copyright holder:
- Smethurst, R
- Copyright date:
- 2016
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