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020 ▼a 9780438019881
035 ▼a (MiAaPQ)AAI10826882
035 ▼a (MiAaPQ)wisc:15364
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 248032
0491 ▼f DP
0820 ▼a 520
1001 ▼a Haines, Tim.
24512 ▼a A Multifaceted Perspective on Galaxy Evolution.
260 ▼a [S.l.] : ▼b The University of Wisconsin - Madison., ▼c 2018
260 1 ▼a Ann Arbor : ▼b ProQuest Dissertations & Theses, ▼c 2018
300 ▼a 124 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B.
500 ▼a Adviser: Elena D'Onghia.
5021 ▼a Thesis (Ph.D.)--The University of Wisconsin - Madison, 2018.
520 ▼a A key component of astronomy is the study of how galaxies change over time. Once thought to be static "island universes" today, we know that galaxies are dynamic systems reacting to changes in their internal and external environments in myriad w
520 ▼a We begin with a simple observation: the stars in our galaxy appear to be moving in strange ways. If our Galaxy were living an uneventful life, we would expect all of the stars to be moving in nearly circular orbits with small, but appreciable, v
520 ▼a Our own galaxy is but one example of an entire population disk-like galaxies with blue colors due to the presence of newly-formed stars. Opposite this population of "blue cloud" galaxies is the "red sequence" which is made up of spheroidal galax
520 ▼a Our understanding of galaxy evolution at every scale relies heavily on computer simulations. In Chapter 4, we approach the subject through the lens of a software developer writing a modern N-body solver used to simulate the gravitational dynamic
590 ▼a School code: 0262.
650 4 ▼a Astronomy.
650 4 ▼a Astrophysics.
690 ▼a 0606
690 ▼a 0596
71020 ▼a The University of Wisconsin - Madison. ▼b Astronomy.
7730 ▼t Dissertation Abstracts International ▼g 79-10B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0262
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998950 ▼n KERIS
980 ▼a 201812 ▼f 2019
990 ▼a 관리자 ▼b 관리자