The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 42 Issue 1
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- Pages.58.4-59
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- 2017
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- 1226-2692(pISSN)
Raman O VI Profile Analysis of Accretion and Bipoloar Outflow in Sanduleak's Star
- Heo, Jeong-Eun (Department of Astronomy and Space Science, Sejong University) ;
- Angeloni, Rodolfo (Gemini Observatory) ;
- Di Mille, Francesco (Las Campanas Observatory) ;
- Palma, Tali (Departamento de Ciencias Fisicas, Universidad Andres Bello) ;
- Lee, Hee-Won (Department of Astronomy and Space Science, Sejong University)
- Published : 2017.04.10
Abstract
Sanduleak's star is a suspected symbiotic binary located in the Large Magellanic Cloud. It is known that it has a giant jet with physical size ~ 14pc. Its spectrum shows two strong emission bands at
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