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020 ▼a 9780438394421
035 ▼a (MiAaPQ)AAI10935460
035 ▼a (MiAaPQ)columbia:14902
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 520
1001 ▼a Hendel, David.
24510 ▼a Dynamics and Detection of Tidal Debris.
260 ▼a [S.l.]: ▼b Columbia University., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 163 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 80-02(E), Section: B.
500 ▼a Adviser: Kathryn V. Johnston.
5021 ▼a Thesis (Ph.D.)--Columbia University, 2018.
520 ▼a Tidal debris structures are striking evidence of hierarchical assembly---the premise that the Milky Way and galaxies like it have been built over cosmic time through the coalescence of many smaller objects. In the prevailing Lambda---Cold Dark M
520 ▼a Around the Milky Way itself we have examined the properties of the Orphan Stream, a stellar tidal stream so named due to uncertainty about the position and current state of its progenitor. Using 3.6 microm observations taken as part of the Spitz
520 ▼a We also examined tidal debris more generally, in particular by investigating the source of the morphological dichotomy between shells and streams. We find that the transition from a stream---like to a shell---like morphology occurs when the diff
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 80-02B(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=T15001194 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033