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020 ▼a 9780438159884
035 ▼a (MiAaPQ)AAI10839133
035 ▼a (MiAaPQ)columbia:14817
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 248032
0820 ▼a 520
1001 ▼a Pearson, Sarah.
24510 ▼a Stellar Streams, Dwarf Galaxy Pairs, and the Halos in Which They Reside.
260 ▼a [S.l.] : ▼b Columbia University., ▼c 2018
260 1 ▼a Ann Arbor : ▼b ProQuest Dissertations & Theses, ▼c 2018
300 ▼a 257 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 79-11(E), Section: B.
500 ▼a Adviser: Kathryn V. Johnston.
5021 ▼a Thesis (Ph.D.)--Columbia University, 2018.
520 ▼a In this Dissertation we explore how the nature of tidal interactions tear gravitationally bound systems apart into distinct morphological and kinematic structures. We use the properties of these structures, persisting for billions of years, to i
520 ▼a In particular, we use the properties of the thin, curved stellar stream emerging from the old, Milky Way globular cluster, Palomar 5 (Pal 5) to show that its mere existence can rule out a moderately triaxial potential model of our Galaxy. Pal 5-
520 ▼a We carry out a systematic study of resolved neutral hydrogen (HI) synthesis maps of 10 interacting dwarf galaxy pairs. The pairs are located in a range of environments and captured at various interaction stages. We find that the neutral gas is e
520 ▼a We model a specific dwarf pair in our sample, NGC 4490/85, which is an isolated analog of the Magellanic Clouds and is surrounded by a &sim
590 ▼a School code: 0054.
650 4 ▼a Astronomy.
650 4 ▼a Astrophysics.
690 ▼a 0606
690 ▼a 0596
71020 ▼a Columbia University. ▼b Astronomy.
7730 ▼t Dissertation Abstracts International ▼g 79-11B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0054
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999672 ▼n KERIS
980 ▼a 201812 ▼f 2019
990 ▼a 관리자