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The Momentum Yield of Clustered SNe
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | The Momentum Yield of Clustered SNe. |
| 개인저자 | Gentry, Eric S. |
| 단체저자명 | University of California, Santa Cruz. Astronomy and Astrophysics (Statistics). |
| 발행사항 | [S.l.]: University of California, Santa Cruz., 2019. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2019. |
| 형태사항 | 306 p. |
| 기본자료 저록 | Dissertations Abstracts International 81-02B. Dissertation Abstract International |
| ISBN | 9781085656177 |
| 학위논문주기 | Thesis (Ph.D.)--University of California, Santa Cruz, 2019. |
| 일반주기 |
Source: Dissertations Abstracts International, Volume: 81-02, Section: B.
Advisor: Madau, Piero. |
| 이용제한사항 | This item must not be sold to any third party vendors. |
| 요약 | Stars are born in clusters and massive stars die relatively quickly, so we expect core collapse supernovae (SNe) to be clustered in both space in time. Despite this, traditional SN feedback models assume SN blasts are isolated and do not interact. In my thesis I show that clustering might have a very large effect on the final momentum added into the SN's host galaxy's interstellar medium (ISM |
| 일반주제명 | Astrophysics. Astronomy. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
