Spectral line Variations of the Symbiotic Variable CH Cygni
(주)코리아스칼라
- 최초 등록일
- 2016.04.02
- 최종 저작일
- 2005.03
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서지정보
ㆍ발행기관 : 한국지구과학회
ㆍ수록지정보 : 한국지구과학회지 / 26권 / 2호
ㆍ저자명 : Yoo, Kye Hwa, Kim, Kang Min, Lee, Byung Chul, Yoon, Tae Seog, Lee, Jung Ae, Kang, Yong Hee
영어 초록
A series of high resolution spectra of CH Cygni obtained at the Bohyunsan Optical Astronomy Observatory (BOAO) in April 2004 has been analyzed. The emission components of the [O I] 6300 A lines are de-convoluted and fitted with Gaussian functions in order to investigate the characteristics and the structure of CH Cygni system along with the analysis for Hα and [O III] lines. A present geometrical structure of the components of CH Cygni system is suggested.
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