The influence of morphology, AGN and environment on the quenching histories of galaxies
thesis by Rebecca Smethurst
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The influence of morphology, AGN and environment on the quenching histories of galaxies
Summary
The influence of morphology, AGN and environment on the quenching histories of galaxies is a doctoral thesis[1].
Key Facts
- The influence of morphology, AGN and environment on the quenching histories of galaxies authored Rebecca Smethurst[2].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's instance of is recorded as doctoral thesis[3].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's publication date is recorded as +2016-12-00T00:00:00Z[4].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's contributor to the creative work or subject is recorded as Chris Lintott[5].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's contributor to the creative work or subject is recorded as Roger Davies[6].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's main subject is recorded as galaxy morphological classification[7].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's main subject is recorded as star formation[8].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's work available at URL is recorded as https://ora.ox.ac.uk/objects/uuid:c7023345-ec69-42c3-907e-32c12a9ee115[9].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's title is recorded as The influence of morphology, AGN and environment on the quenching histories of galaxies[10].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's thesis submitted to is recorded as University of Oxford[11].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's EThOS thesis ID is recorded as uk.bl.ethos.730234[12].
- The influence of morphology, AGN and environment on the quenching histories of galaxies's copyright status is recorded as copyrighted[13].
Body
Designation and Status
The influence of morphology, AGN and environment on the quenching histories of galaxies's instance of is recorded as doctoral thesis[3].