| LDR | | 01992nmm uu200421 4500 |
| 001 | | 000000331765 |
| 005 | | 20240805165322 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438394421 |
| 035 | |
▼a (MiAaPQ)AAI10935460 |
| 035 | |
▼a (MiAaPQ)columbia:14902 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 520 |
| 100 | 1 |
▼a Hendel, David. |
| 245 | 10 |
▼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. |
| 502 | 1 |
▼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 |
| 710 | 20 |
▼a Columbia University.
▼b Astronomy. |
| 773 | 0 |
▼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 |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T15001194
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |