| LDR | | 01826nmm uu200409 4500 |
| 001 | | 000000333949 |
| 005 | | 20240805174837 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438205802 |
| 035 | |
▼a (MiAaPQ)AAI10826813 |
| 035 | |
▼a (MiAaPQ)wisc:15363 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 520 |
| 100 | 1 |
▼a Kundert, Alisha R. |
| 245 | 10 |
▼a Exploring the Nature of Fossil Galaxy Systems with Simulations and X-ray Observations. |
| 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 135 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-12(E), Section: B. |
| 500 | |
▼a Adviser: Elena D'Onghia. |
| 502 | 1 |
▼a Thesis (Ph.D.)--The University of Wisconsin - Madison, 2018. |
| 520 | |
▼a Fossil galaxy groups and clusters are characterized by an extreme difference in brightness between their central and satellite galaxies. This magnitude gap has been proposed to form as the result of significant mergers of massive satellite galax |
| 520 | |
▼a In this thesis, the properties of fossil systems are first examined by constructing the global optical and X-ray scaling relations of fossils across the group and cluster mass regimes. Then, using the Illustris cosmological simulation, the mass |
| 590 | |
▼a School code: 0262. |
| 650 | 4 |
▼a Astronomy. |
| 650 | 4 |
▼a Astrophysics. |
| 690 | |
▼a 0606 |
| 690 | |
▼a 0596 |
| 710 | 20 |
▼a The University of Wisconsin - Madison.
▼b Astronomy. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-12B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0262 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998942
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |