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Fuel for the Star Formation Engine: Dense Molecular Cloud Clumps in the Northern Galactic Plane
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| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | Fuel for the Star Formation Engine: Dense Molecular Cloud Clumps in the Northern Galactic Plane. |
| 개인저자 | Zetterlund, Erika. |
| 단체저자명 | University of Colorado at Boulder. Astrophysical and Planetary Sciences. |
| 발행사항 | [S.l.]: University of Colorado at Boulder., 2018. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2018. |
| 형태사항 | 204 p. |
| 기본자료 저록 | Dissertation Abstracts International 80-02B(E). Dissertation Abstract International |
| ISBN | 9780438382176 |
| 학위논문주기 | Thesis (Ph.D.)--University of Colorado at Boulder, 2018. |
| 일반주기 |
Source: Dissertation Abstracts International, Volume: 80-02(E), Section: B.
Adviser: Jason Glenn. |
| 요약 | The interstellar medium (ISM) is a confusing, muddled place. It provides the fuel for star formation, but before that can occur, the ISM must cool and condense into molecular clouds. Even this is not enough, however. It is only the cores, contai |
| 요약 | I use the Herschel infrared GALactic plane survey (Hi-GAL) to study molecular cloud clumps through their thermal dust emission at 500 microm. For adapting and testing the clump identification and distance techniques---developed for the Bolocam G |
| 요약 | The application of these techniques to 10° < &ell |
| 요약 | Finally, with the addition of a catalog of clouds produced using the CO High Resolution Survey (COHRS), I addressed molecular cloud clumps as fuel for star formation. I matched 3,674 clumps from my catalog to 473 clouds from the COHRS catalog, a |
| 일반주제명 | Astrophysics. Physics. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
