Hostname: page-component-745bb68f8f-cphqk Total loading time: 0 Render date: 2025-01-13T06:14:05.806Z Has data issue: false hasContentIssue false
  • English
  • Français

Ultraviolet Fe II Absorption Lines in HD 59643

Published online by Cambridge University Press:  12 April 2016

Joel A. Eaton
Joel A. Eaton*
Affiliation:
Indiana UniversityBloominton, IN, U.S.A

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
Session 1. The Basic Data
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 25 - 26
Copyright
Copyright © Kluwer 1988

References

Ake, T.B., and Johnson, H.R. 1987, Ap. J., in preparation.Google Scholar
Che, A., Hempe, K., and Reimers, D. 1983, Astron. Ap., 126, 225.Google Scholar
Eaton, J.A., and Barden, S.J. 1987, in preparation.Google Scholar
Hutchings, J.B., Cowley, A.P., Ake, T.B., and Imhoff, C.L. 1983, Ap. J., 275, 271.CrossRefGoogle Scholar
Kondo, Y., McCluskey, G.E., and Parsons, S.B. 1985, Ap. J., 295, 580 Google Scholar
Kurucz, R.L. 1981, S. A. O. Special Report, No. 390.Google Scholar
Plavec, M.J., and Dobias, J.J. 1987, A. J., 93, 440.Google Scholar
Plavec, M.J., Weiland, J.L., and Koch, K.H. 1982, Ap. J., 256, 206.CrossRefGoogle Scholar
Querci, M.F., Johnson, H.R., and Baumert, J.H. 1986, Adv.Space Res., 6, 215.CrossRefGoogle Scholar