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The Shape and Dynamics of Galaxy Clu...

Shin, Tae-hyeon.

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The Shape and Dynamics of Galaxy Clusters and Evolution of Their Satellite Galaxies.

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	The Shape and Dynamics of Galaxy Clusters and Evolution of Their Satellite Galaxies./
作者:	Shin, Tae-hyeon.
出版者:	Ann Arbor : ProQuest Dissertations & Theses, : 2020,
面頁冊數:	190 p.
附註:	Source: Dissertations Abstracts International, Volume: 81-11, Section: B.
Contained By:	Dissertations Abstracts International81-11B.
標題:	Astrophysics. -
電子資源:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=27956662
ISBN:	9798645424794

The Shape and Dynamics of Galaxy Clusters and Evolution of Their Satellite Galaxies.
Shin, Tae-hyeon.

The Shape and Dynamics of Galaxy Clusters and Evolution of Their Satellite Galaxies. - Ann Arbor : ProQuest Dissertations & Theses, 2020 - 190 p.

Source: Dissertations Abstracts International, Volume: 81-11, Section: B.

Thesis (Ph.D.)--University of Pennsylvania, 2020.

This item must not be sold to any third party vendors.

Galaxy clusters, which originate from the highest density peaks in the primordial Universe, contain valuable information on cosmology. They are fascinating objects in their own right as they involve an interplay of the physics of dark matter, gas and galaxies. Their complex formation history also leaves observational imprints. We study the shape and the boundary of galaxy clusters and their implications for astrophysics and cosmology. The evolution and dynamics of galaxies in cluster environments are two of the main applications studied in this thesis.

ISBN: 9798645424794Subjects--Topical Terms:

535904
Astrophysics.
Subjects--Index Terms:

Cosmology

The Shape and Dynamics of Galaxy Clusters and Evolution of Their Satellite Galaxies.
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300 $a 190 p.
500 $a Source: Dissertations Abstracts International, Volume: 81-11, Section: B.
500 $a Advisor: Jain, Bhuvnesh.
502 $a Thesis (Ph.D.)--University of Pennsylvania, 2020.
506 $a This item must not be sold to any third party vendors.
520 $a Galaxy clusters, which originate from the highest density peaks in the primordial Universe, contain valuable information on cosmology. They are fascinating objects in their own right as they involve an interplay of the physics of dark matter, gas and galaxies. Their complex formation history also leaves observational imprints. We study the shape and the boundary of galaxy clusters and their implications for astrophysics and cosmology. The evolution and dynamics of galaxies in cluster environments are two of the main applications studied in this thesis.
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653 $a Dark matter
653 $a Ellipticity
653 $a Galaxy cluster
653 $a Splashback
653 $a Weak-lensing
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793 $a English
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