Abstract
The Balmer lines of interacting binaries cannot be interpreted in the usual sense as diagnostics of stellar photospheres. In an Algol-type binary, the presence of circumstellar material can lead to inconsistent interpretations about the nature of the hotter stellar component. The system TT Hydrae has fairly well established stellar properties. Its Balmer—line spectrum illustrates complications from circumstellar material. Complications at Hα because of the cooler secondary are also evident. Failure to recognize this complication could result in misinterpretations about the circumstellar material.
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References
Allen, C.W. (1973). Astrophysical Quantities, third edition, ( Athlone, London).
Batten, A. H. (1988). Publ. Astron. Soc. Pac. 100, 160.
BideIman, W.P. (1976). In Be and Shell Stars, edited by A. Slettebak, ( Reidel Publ., Dordrecht ), p. 457.
Etzel, P.B. (1984). Bull. Amer. Astron. Soc. 16, 504.
Etzel, P.B. (1988). Astron. J. 95, 1204.
Etzel, P.B. (1989a). “Spectrophotometry of Algol-Type Binaries” In Active Close Binaries, edited by C. Ibanoglu and I. Yavuz, (these proceedings).
Etzel, P.B. (1989b). Publ. Astron. Soc. Pac. (in preparation).
Groth, H.-G. (1961) Z. Astrophys. 51, 231.
Harmanec, P. (1982). In Be Stars, edited by M. Jaschek and H.-G. Groth, ( Reidel Publ., Dordrecht ), p. 279.
Joy, A. H. (1942). Publ. Astron. Soc. Pac. 54, 35.
Joy, A. H. (1988). Publ. Astron. Soc. Pac. 100, 157.
Kaitchuck, R. H., and Honeycutt, R. K. (1982). Astrophys. J. 258, 224.
Kaitchuck, R. H., and Honeycutt, R. K. and Schlegel, E. M. (1985). Publ. Astron. Soc. Pac. 97, 1178.
Kurucz, R. L. (1979). Astrophys. J. Suppl. 40, 1.
Lubow, S. H., and Shu, F. H. (1975). Astrophys. J. 198, 383.
Naftilan, S. A. (1975). Publ. Astron. Soc. Pac. 87, 321.
Peters, G. J. (1980). In Close Binary Stars: Observations and Interpretations, edited by M. J. Plavec, D. M. Popper, and R. K. Ulrich, ( Reidel Publ., Dordrecht ), p. 287.
Peters, G. J. (1989). Space Science Reviews 50, 9.
Peters, G. J., and Polidan, R. S. (1984). Astrophys. J. 283, 745.
Plavec, M. J. (1976). In Be and Shell Stars, edited by A. Slettebak,
Plavec, M. J. (1983). Astrophys. J. 275, 251.
Plavec, M. J. (1988). Astron. J. 96, 755.
Popper, D. M. (1980). Annu. Rev. Astron. Astrophys. 18, 115.
Popper, D. M. (1982). Publ. Astron. Soc. Pac. 94, 945.
Popper, D. M. (1989). Astrophys. J. Suppl. (in press).
Sahade, J., and Cesco, C. U. (1946). Astrophys. J. 139, 793.
Wyse, A. B. (1934). Lick Obs. Bull. 17, 37.
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© 1990 Kluwer Academic Publishers
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Etzel, P.B. (1990). Complications in the Balmer-Line Spectrum of TT Hydrae. In: İbanoğlu, C. (eds) Active Close Binaries. NATO ASI Series, vol 319. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0679-2_15
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DOI: https://doi.org/10.1007/978-94-009-0679-2_15
Publisher Name: Springer, Dordrecht
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