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Author ORCID Identifier
https://orcid.org/0000-0001-7673-2257
AccessType
Campus-Only Access for Five (5) Years
Degree Name
Doctor of Philosophy (PhD)
Degree Program
Astronomy
Year Degree Awarded
2060
Month Degree Awarded
February
First Advisor
Zhiyuan Ji
Subject Categories
Cosmology, Relativity, and Gravity | External Galaxies | Physical Processes
Abstract
Observations both in the local universe and at high redshift have clearly shown that galaxies are characterized by a distinct bimodality of star-formation and structural properties and that is reflected in a corresponding bimodality of colors, morphology types, and specific star formation rates. Particular attention has been devoted to the so-called galaxy quenching, which refers to the sets of processes that shut down the star formation activity inside galaxies and drive the transformation of galaxies from one type of the bimodality to the other, i.e., from a star-forming galaxy to a quiescent one. The physics of quenching remains a key missing piece toward a complete picture of galaxy evolution. This thesis is broadly concerned with investigating the joint evolution of super massive black hole, star-formation and structural properties of galaxies across cosmic times, with the goal of empirically constraining the physics of galaxy quenching at cosmic noon epoch.
DOI
https://doi.org/10.7275/31907070
Recommended Citation
"The Physics of Galaxy Quenching at Cosmic Noon Epoch" (2023). Doctoral Dissertations. 2759.
https://doi.org/10.7275/31907070
https://scholarworks.umass.edu/dissertations_2/2759
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.