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008181129s2018 ||| | | | eng d
020 ▼a 9780438353725
035 ▼a (MiAaPQ)AAI10842298
035 ▼a (MiAaPQ)umn:19484
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 248032
0491 ▼f DP
0820 ▼a 520
1001 ▼a Gordon, Michael Scott.
24510 ▼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
5021 ▼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
71020 ▼a University of Minnesota. ▼b Astrophysics.
7730 ▼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
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14999840 ▼n KERIS
980 ▼a 201812 ▼f 2019
990 ▼a 관리자 ▼b 관리자