Abstract
The analysis of the spectrum of emission line stars in a wide spectral range has put in evidence a number of high excitation emission lines having anomalously high intensities. We illustrate the case of the high excitation Fe II lines observed in the ultraviolet and near—IR of different stellar categories, and discuss the information which can be derived from their study.
Based on observations collected at OHP (France) and LNA (Brazil)
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References
Damineli A., Cassatella A., Viotti R., et al. (1995), Rev. Mex. A. Ap., 2, 41
Hamann F., DePoy D.L., Johansson S., Elias J. (1994), ApJ, 422, 626
Kurucz R.L. (1981), Srnithonian Astrophys. Obs. Special Report, 390
Johansson S. (1984) Phys. Scripta, T8, 63
Muratorio G., Viotti R., Friedjung M., et al. (1992), A &A, 258, 423
Torres R.M. (1994), Master Thesis, IAGUSP, São Paulo, Brazil
Viotti R. (1976), ApJ, 204, 293
Viotti R., Rossi L., Cassatella A., et al. (1989), ApJS, 71, 983
Viotti R., Rossi C., Muratorio G. (1997), A&AS in press
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© 1998 Springer Science+Business Media Dordrecht
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Viotti, R., Damineli, A., Rossi, C. (1998). The High Excitation Fe II Lines as a Diagnostics of the Outer Envelopes of Early Type Emission Line Stars. In: Hubert, A.M., Jaschek, C. (eds) B[e] Stars. Astrophysics and Space Science Library, vol 233. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9014-3_7
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DOI: https://doi.org/10.1007/978-94-015-9014-3_7
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-5080-9
Online ISBN: 978-94-015-9014-3
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