| LDR | | 01577nmm uu200421 4500 |
| 001 | | 000000333363 |
| 005 | | 20240805172904 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438116818 |
| 035 | |
▼a (MiAaPQ)AAI10816660 |
| 035 | |
▼a (MiAaPQ)northwestern:14138 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Breivik, Katelyn.
▼0 (orcid)0000-0001-5228-6598 |
| 245 | 10 |
▼a Simulating Binary Populations in the Milky Way. |
| 260 | |
▼a [S.l.] :
▼b Northwestern University.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 124 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-11(E), Section: B. |
| 500 | |
▼a Adviser: Shane L. Larson. |
| 502 | 1 |
▼a Thesis (Ph.D.)--Northwestern University, 2018. |
| 520 | |
▼a The most promising probe into compact binary formation and evolution will be the populations resolved by both gravitational wave (GW) and electromagnetic (EM) observatories. As with any observation, theoretical models must be characterized to ga |
| 590 | |
▼a School code: 0163. |
| 650 | 4 |
▼a Astrophysics. |
| 650 | 4 |
▼a Physics. |
| 650 | 4 |
▼a Astronomy. |
| 690 | |
▼a 0596 |
| 690 | |
▼a 0605 |
| 690 | |
▼a 0606 |
| 710 | 20 |
▼a Northwestern University.
▼b Physics and Astronomy. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-11B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0163 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998275
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |