| LDR | | 01841nam u200409 4500 |
| 001 | | 000000418469 |
| 005 | | 20190215162904 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438353725 |
| 035 | |
▼a (MiAaPQ)AAI10842298 |
| 035 | |
▼a (MiAaPQ)umn:19484 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 247004 |
| 082 | 0 |
▼a 520 |
| 100 | 1 |
▼a Gordon, Michael Scott. |
| 245 | 10 |
▼a Massive Stars: An Infrared Exploration across the HR Diagram. |
| 260 | |
▼a [S.l.]:
▼b University of Minnesota.,
▼c 2018. |
| 260 | 1 |
▼a Ann Arbor:
▼b ProQuest Dissertations & Theses,
▼c 2018. |
| 300 | |
▼a 120 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 80-01(E), Section: B. |
| 500 | |
▼a Advisers: Terry J. Jones |
| 502 | 1 |
▼a Thesis (Ph.D.)--University of Minnesota, 2018. |
| 520 | |
▼a The main goal of this dissertation is to understand how stellar winds, dusty ejecta, and overall mass-loss histories affect the end-stage evolution of supergiant stars. To what extent mass loss and periods of enhanced stellar outflow can influen |
| 520 | |
▼a Here, we focus on characterizing the circumstellar (CS) ejecta around supergiants through a combination of observing techniques. Over the last several years, using the Large Binocular Telescope (LBT), MMT, NASA's Infrared Telescope Facility (IRT |
| 590 | |
▼a School code: 0130. |
| 650 | 4 |
▼a Astronomy. |
| 650 | 4 |
▼a Astrophysics. |
| 690 | |
▼a 0606 |
| 690 | |
▼a 0596 |
| 710 | 20 |
▼a University of Minnesota.
▼b Astrophysics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 80-01B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0130 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999840
▼n KERIS
▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a ***1012033 |