| LDR | | 01631nmm uu200421 4500 |
| 001 | | 000000332568 |
| 005 | | 20240805171032 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438063716 |
| 035 | |
▼a (MiAaPQ)AAI10788864 |
| 035 | |
▼a (MiAaPQ)unc:17690 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Frazer, Christopher Charles. |
| 245 | 10 |
▼a Gas Dynamics and Star Formation Near Supermassive Black Holes. |
| 260 | |
▼a [S.l.] :
▼b The University of North Carolina at Chapel Hill.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 148 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B. |
| 500 | |
▼a Adviser: Fabian Heitsch. |
| 502 | 1 |
▼a Thesis (Ph.D.)--The University of North Carolina at Chapel Hill, 2018. |
| 520 | |
▼a The existence of young stars in the central parsec of the Milky Way's Galactic Center (GC) is challenging to explain due to the extreme tidal field of the supermassive black hole (SMBH), Sgr A*, which is expected to disrupt any potentially star |
| 590 | |
▼a School code: 0153. |
| 650 | 4 |
▼a Astrophysics. |
| 650 | 4 |
▼a Astronomy. |
| 650 | 4 |
▼a Fluid mechanics. |
| 690 | |
▼a 0596 |
| 690 | |
▼a 0606 |
| 690 | |
▼a 0204 |
| 710 | 20 |
▼a The University of North Carolina at Chapel Hill.
▼b Physics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-10B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0153 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14997476
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |