- 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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Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
- Department:
- Physics
- Role:
- Supervisor
- Department:
- Physics
- Role:
- Examiner
- Department:
- University of Hull
- Role:
- Examiner
- Grant:
- ST/K502236/1
- Funding agency for:
- Rebecca Smethurst
- Type of award:
- DPhil
- Level of award:
- Doctoral
- Awarding institution:
- University of Oxford
- Language:
- English
- Keywords:
- Subjects:
- Copyright date:
- 2016
Thesis
The influence of morphology, AGN and environment on the quenching histories of galaxies
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Authors
Contributors
+ Chris Lintott
+ Roger Davies
+ Kevin Pimblett
Funding
+ Science and Technology Facilities Council
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