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The Algols, Red Spectra, Be Stars, and Even Neutrinos

Published online by Cambridge University Press:  14 August 2015

M. Plavec  and
R. S. Polidan
M. Plavec
Affiliation:
Dept. of Astronomy, University of California, Los Angeles, Calif., U.S.A.
R. S. Polidan
Affiliation:
Dept. of Astronomy, University of California, Los Angeles, Calif., U.S.A.

Abstract

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The introduction of image tubes makes spectroscopic studies in the red and near infrared spectral regions much more efficient. Work currently done at the Lick Observatory by the Los Angeles binary star investigators is reported. Preliminary results on element abundances in the subgiant in U Sagittae indicate that there may indeed exist systematic abundance anomalies of potential relevance to the problem of the solar neutrino flux. Emission at Hα has been observed in many systems, and several types of circumstellar features are indicated. It is suggested that some Be stars and shell stars are interacting binaries. The possibility of observing very deep stellar eclipses is discussed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 73: Structure and Evolution of Close Binary Systems , 1976 , pp. 289 - 302
Copyright
Copyright © Reidel 1976 

References

Bahcall, J. N. and Ulrich, R. K.: 1971, Astrophys. J. 170, 593.CrossRefGoogle Scholar
Baldwin, B. W.: 1973, Publ. Astron. Soc. Pacific 85, 714.CrossRefGoogle Scholar
Batten, A. H., Fisher, W. A., Baldwin, B. W., and Scarfe, C. D.: 1974, Nature 253, 174.CrossRefGoogle Scholar
Bodenheimer, P. and Ostriker, J. P.: 1970, Astrophys. J. 161, 1101.Google Scholar
Bond, H. E.: 1972, Publ. Astron. Soc. Pacific 84, 839.Google Scholar
Cowley, A. P.: 1967, Astrophys. J. 148, 667.CrossRefGoogle Scholar
Crawford, R. C. and Plavec, M.: 1975, Bull. Amer. Astron. Soc. 7, 462.Google Scholar
Doremus, C.: 1970, Publ. Astron. Soc. Pacific 82, 745.CrossRefGoogle Scholar
Gaposchkin, S.: 1946, Harvard Bull. , 918.Google Scholar
Hack, M., Hutchings, J. B., Kondo, Y., McCluskey, G. E., Plavec, M., and Polidan, R. S.: 1975, Astrophys. J. 198, 453.CrossRefGoogle Scholar
Hall, D. S.: 1967, Astron. J. 72, 301.Google Scholar
Hall, D. S.: 1971, Bamberg Variable Star Colloq. , p. 217.Google Scholar
Hall, D. S.: 1974, Acta Astron. 24, 215.Google Scholar
Joy, A. H.: 1930, Astrophys. J. 71, 336.CrossRefGoogle Scholar
Joy, A. H.: 1942, Publ. Astron. Soc. Pacific 54, 35.Google Scholar
Koch, R. H.: 1960, Astron. J. 65, 139.Google Scholar
Koch, R. H.: 1972, Publ. Astron. Soc. Pacific 84, 5.Google Scholar
Koch, R. H.: 1973, Astron. J. 78, 410.Google Scholar
Kopal, Z.: 1959, Close Binary Systems , Chapman and Hall, chap. VII.Google Scholar
Křiž, S.: 1971, Bull. Astron. Czech. 22, 108.Google Scholar
Křiž, S. and Harmanec, P.: 1975, Bull. Astron. Czech. 26, 65.Google Scholar
Lubow, S. H. and Shu, F. H.: 1975, Astrophys. J. 198, 383.CrossRefGoogle Scholar
Marlborough, J. M.: 1969, Astrophys. J. 156, 135.Google Scholar
Marlborough, J. M. and Cowley, A. P.: 1974, Astrophys. J. 187, 99.Google Scholar
McNamara, D. H.: 1967, Astrophys. J. 149, 723.Google Scholar
Miner, E. D.: 1966, Astrophys. J. 144, 1101.CrossRefGoogle Scholar
Naftilan, S. A.: 1975a, Publ. Astron. Soc. Pacific 87, 321.CrossRefGoogle Scholar
Naftilan, S. A.: 1975b, Bull. Amer. Astron. Soc. 7, 476.Google Scholar
Plavec, M.: 1970, in Slettebak, A. (ed.), Stellar Rotation , D. Reidel Publ. Co., Dordrecht, Holland, p. 133.Google Scholar
Plavec, M.: 1973, IAU Symp. 51, 216.Google Scholar
Plavec, M. and Horn, J.: 1969, in Hack, M. (ed.), Mass Loss from Stars , D. Reidel Publ. Co., Dordrecht, Holland, p. 242.CrossRefGoogle Scholar
Plavec, M. and Polidan, R. S.: 1974, Nature 253, 173.Google Scholar
Polidan, R. S.: 1975, Bull. Amer. Astron. Soc. 7, 451.Google Scholar
Popper, D. M.: 1973, Astrophys. J. 185, 265.Google Scholar
Popper, D. M. and Plavec, M.: 1974, Bull. Amer. Astron. Soc. 6, 334.Google Scholar
Popper, D. M. and Plavec, M.: 1976, Astrophys. J. 205, 462.Google Scholar
Refsdal, S., Roth, M. L., and Weigert, A.: 1974, Astron. Astrophys. 36, 113.Google Scholar
Struve, O.: 1950, Stellar Evolution , Princeton Univ. Press, p. 27.CrossRefGoogle Scholar
Ulrich, R. K.: 1974, in Baltay, C. (ed.), Neutrinos 1974 , Amer. Inst. of Physics, p. 259.Google Scholar
van de Heuvel, E. P. J.: 1970, in Slettebak, A. (ed.), Stellar Rotation , D. Reidel Publ. Co., Dordrecht, Holland, p. 178.Google Scholar
Wilson, R. E.: 1972, Astrophys. Space Sci. 19, 165.Google Scholar