Abstract
This report is concerned with spectroscopic diagnoses on the gaseous region of symbiotic stars based upon our recent work(Ikeda and Tamura, 1999: submitted to P.A.S.Japan). It is now widely accepted that the symbiotic star is a binary system which consists of a cool giant and a hot dwarf surrounded or accompanied with the ionized gas, probably together with dusts. Usually we can not recognize a hot star in the spectrum directly. Therefore, it looks like that a cool giant coexist with the ionized gas which produce rich emission-lines. This is the origin of the designation as symbiotic stars.
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© 2000 Springer Science+Business Media Dordrecht
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Tamura, S., Ikeda, Y. (2000). Symbiotic Stars with Highly Resolved Emission Line Profiles. In: Cheng, K.S., Chau, H.F., Chan, K.L., Leung, K.C. (eds) Stellar Astrophysics. Astrophysics and Space Science Library, vol 254. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0878-5_35
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DOI: https://doi.org/10.1007/978-94-010-0878-5_35
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3791-4
Online ISBN: 978-94-010-0878-5
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