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Ultraviolet FE II Absorption Lines in HD 59643

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The Symbiotic Phenomenon

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 145))

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Abstract

The peculiar red giant HD 59643 (C6,2) has a composite spectrum like a symbiotic star’s except for the absence of highly ionized species. UV observations show a highly variable hot continuum with superimposed absorptions of Fe II and the common emission lines of C IV, Si III], C III], C II], and Mg II. These Fe II absorptions, which are practically ubiquitous in interacting binaries, are an effective diagnostic of turbulence and distribution of scattering gas, even at low resolution.

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© 1988 Kluwer Academic Publishers

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Eaton, J.A. (1988). Ultraviolet FE II Absorption Lines in HD 59643. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_4

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  • DOI: https://doi.org/10.1007/978-94-009-2969-2_4

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7833-7

  • Online ISBN: 978-94-009-2969-2

  • eBook Packages: Springer Book Archive

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