천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제37권1호
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- Pages.73.2-73.2
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- 2012
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- 1226-2692(pISSN)
Dust-scattered FUV halo around Spica
- Choi, Yeon-Ju (Korea Advanced Institute of Science and Technology) ;
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Min, Kyoung-Wook
(Korea Advanced Institute of Science and Technology) ;
- Park, Jae-Woo (Korean Intellectual Property Office) ;
- Lim, Tae-Ho (Korea Advanced Institute of Science and Technology) ;
- Seon, Kwang-Il (Korea Astronomy and Space Science Institute)
- 발행 : 2012.04.03
초록
The far ultraviolet (FUV) wavelength (900-1750A) range includes a wealth of important astrophysical information related to the cooling of hot gas, fluorescent emission from H2 molecules, and starlight scattered off dust particles. Among these, we would like to focus on the scattered emission of the central star by dust with the example of the FUV halo surrounding
키워드