Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-27T00:43:36.705Z Has data issue: false hasContentIssue false
  • English
  • Français

Duplicity of Be Stars as Seen from Ondřejov: (Review Paper)

Published online by Cambridge University Press:  14 August 2015

Petr Harmanec  and
Svatopluk Kříž
Petr Harmanec
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
Svatopluk Kříž
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia

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.

Observed Be stars are considered to be interacting binaries undergoing mostly case B mass exchange. Their observed properties can be explained satisfactorily as the consequences of different modes of mass transfer. Suggestions for further observational and theoretical studies to verify or to disprove the hypothesis presented here are briefly outlined.

Type
Part VI: Single Versus Binary Stars
Information
Symposium - International Astronomical Union , Volume 70: Be and Shell Stars , 1976 , pp. 385 - 400
Copyright
Copyright © Reidel 1976 

References

Albert, E. and Huang, S.-S.: 1974, Astrophys. J. 189, 479.CrossRefGoogle Scholar
Batten, A. H.: 1967, Publ. Dominion Astrophys. Obs. 13, 119.Google Scholar
Batten, A. H.: 1968, J. Roy. Astron. Soc. Can. 62, 344.Google Scholar
Batten, A. H.: 1974, Publ. Dominion Astrophys. Obs. 14, 191.Google Scholar
Biermann, P. and Hall, D. S.: 1973, Astron. Astrophys. 27, 249.Google Scholar
Cowley, A. P.: 1964, Astrophys. J. 139, 817.CrossRefGoogle Scholar
Delplace, A. M.: 1970, Astron. Astrophys. 7, 68.Google Scholar
Doazan, V.: 1973, Astron. Astrophys. 27, 395.Google Scholar
Haefner, R., Metz, K., and Schoembs, R.: 1975, Astron. Astrophys. 38, 203.Google Scholar
Hall, D. S.: 1975, Acta Astron. 25, 1.Google Scholar
Hall, D. S. and Garrison, L. M.: 1972, Publ. Astron. Soc. Pacific 84, 552.CrossRefGoogle Scholar
Harmanec, P.: 1976, to be published.Google Scholar
Harmanec, P., Koubsky, P., and Krpata, J.: 1972a, Bull. Astron. Inst. Czech. 23, 218.Google Scholar
Harmanec, P., Koubsky, P., and Krpata, J.: 1972b, Astrophys. Letters 11, 119.Google Scholar
Harmanec, P., Koubsky, P., and Krpata, J.: 1973, Astron. Astrophys. 22, 337.Google Scholar
Harmanec, P., Koubsky, P., and Krpata, J.: 1974, Astron. Astrophys. 33, 117.Google Scholar
Harmanec, P., Koubsky, P., Krpata, J., and Žďársky, F.: 1976, Bull. Astron. Inst. Czech. 27, 47.Google Scholar
Heard, J. F., Hurkens, R., Harmanec, P., Koubsky, P., and Krpata, J.: 1975, Astron. Astrophys. 42, 47.Google Scholar
Huang, S.-S.: 1973, Astrophys. J. 183, 541.CrossRefGoogle Scholar
Hutchings, J. B., Auman, J. R., Gower, A. C., and Walker, G. A. H.: 1971, Astrophys. J. 170, L73.Google Scholar
Hutchings, J. B. and Redman, R. O.: 1973, Monthly Notices Roy. Astron. Soc. 163, 209.Google Scholar
Hynek, J. A. and Struve, O.: 1942, Astrophys. J. 96, 425.Google Scholar
Kříž, S.: 1969, in Hack, M. (ed.), Mass Loss from Stars , D. Reidel Publ. Co., Dordrecht-Holland, p. 257 Google Scholar
Kříž, S.: 1973, Nature 245, 36.Google Scholar
Kříž, S. and Harmanec, P.: 1975, Bull. Astron. Inst. Czech. 26, 65.Google Scholar
Lester, D. F.: 1975, Publ. Astron. Soc. Pacific 87, 177.Google Scholar
Lubow, S. H. and Shu, F. H.: 1975, Astrophys. J. 198, 383.Google Scholar
Lynds, C. R.: 1957, Astrophys. J. 126, 81.Google Scholar
Lynds, C. R.: 1960, Astrophys. J. 131, 390.Google Scholar
Magalashvili, N. L. and Kumsishvili, J. I.: 1969, Bull. Abastumani , No. 37.Google Scholar
McLaughlin, D. B.: 1961, J. Roy. Astron. Soc. Can. 55, 13 and 73.Google Scholar
Nordh, L. and Olofsson, G.: 1974, Stockholm Obs. Report , No. 7.Google Scholar
Paczynski, B.: 1971, Ann. Rev. Astron Astrophys. 9, 183.Google Scholar
Peters, G. J.: 1973, in Batten, A. H. (ed.), ‘Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems’, IAU Symp. 51, 174.Google Scholar
Plavec, M.: 1970a, Publ. Astron. Soc. Pacific 82, 957.Google Scholar
Plavec, M.: 1970b, in Slettebak, A. (ed.), Stellar Rotation , D. Reidel Publ. Co., Dordrecht-Holland, p. 133.CrossRefGoogle Scholar
Plavec, M.: 1973, in Batten, A. H. (ed.), ‘Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems’, 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.Google Scholar
Plavec, M., Polidan, R. S., and Peters, G. J.: 1973a, A paper presented at the 141st meeting of AAS.Google Scholar
Plavec, M., Ulrich, R. K., and Polidan, R. S.: 1973b, Publ. Astron. Soc. Pacific 85, 769.Google Scholar
Polidan, R. S., Peters, G. J., and Plavec, M.: 1973, A paper presented at the 141st meeting of AAS.Google Scholar
Prendergast, K. H. and Taam, R. E.: 1974, Astrophys. J. 189, 125.Google Scholar
Ringuelet, A. E. and Machado, M. E.: 1974, Astrophys. J. 189, 285.Google Scholar
Struve, O.: 1931, Astrophys. J. 73, 94.CrossRefGoogle Scholar
Struve, O.: 1944a, Astrophys. J. 99, 89.Google Scholar
Struve, O.: 1944b, Astrophys. J. 99, 75.Google Scholar
Thackeray, A. D.: 1971, Monthly Notices Roy. Astron. Soc. 154, 103.Google Scholar
Van den Heuvel, E. P. J. and De Loore, C.: 1973, Astron. Astrophys. 25, 387.Google Scholar
Walker, M. F.: 1953, Astrophys. J. 118, 481.CrossRefGoogle Scholar
Wilson, R. E. and Stothers, R.: 1975, Monthly Notices Roy. Astron. Soc. 170, 497.Google Scholar
Woolf, N. J.: 1962, Monthly Notices Roy. Astron. Soc. 123, 399.Google Scholar