The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 37 Issue 1
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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) ;
- 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)
- Published : 2012.04.03
Abstract
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
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