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Emission-Line Stars as Interacting Binaries (Review Paper)

Published online by Cambridge University Press:  23 September 2016

P. Harmanec

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A general binary hypothesis of the emission-line phenomenon in early-type stars was published eleven years ago (Kříž & Harmanec 1975, Harmanec & Kříž 1976; for a reformulation see Harmanec 1982). Since then, new observational techniques and theoretical concepts have led to a number of exciting findings which have made the emission-line phenomenon even more puzzling and challenging than before. It is therefore of interest to ask whether the binary hypothesis can withstand all these developments or not.

Type
IV. Models
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 339 - 360
Copyright
Copyright © Cambridge University Press 1987

References

Abt, H.A. & Biggs, E.S. (1972). Bibliography of Stellar Radial Velocities. New York: Latham Process Corp. Google Scholar
Abt, H.A. & Cardona, O. (1984). Astrophys.J. 285, 190.Google Scholar
Baade, D. (1979). Unpublished Thesis, Astron. Inst., Univ. Munster.Google Scholar
Baade, D. (1982a). Astron. Astrophys. 105, 65.Google Scholar
Baade, D. (1982b). Astron. Astrophys. 110, L15.Google Scholar
Baade, D. (1984), Astron. Astrophys. 134, 105.Google Scholar
Baade, D. (1985). Astron. Astrophys. 148, 59.Google Scholar
Balona, L.A. & Engelbrecht, C.A. (1986). Mon.Not.Roy.Astron.Soc. 219, 131.CrossRefGoogle Scholar
Barr, J.M. (1908), J.Roy.Astron.Soc.Canada, 2, 70.Google Scholar
Bath, G.T. & Paradijs van, J. (1983). Nature 305, 33.Google Scholar
Biermann, P. & Hall, D.S. (1973). Astron. Astrophys. 27, 249.Google Scholar
Bolton, C.T. (1982). IAU Symp. 98, 181.Google Scholar
Bolton, C.T., Fullerton, A., Bohlender, D., Landstreet, J.D. & Gies, D.R. (1986). These Proceedings.Google Scholar
Bopp, B.W. (1983). In Activity in Red-Dwarf Stars, ed. Byrne, P.B. & Rodono, M., p. 363. Dordrecht: D. Reidel.Google Scholar
Clarke, D. & McGale, P.A. (1986). These Proceedings.Google Scholar
Cowley, A. & Gugula, E. (1973). Astron. Astrophys. 22, 283.Google Scholar
Doazan, V. & Thomas, R.N. (1982). In B Stars with and without Emission Lines, ed. Underhill, A. & Doazan, V., p.409. NASA SP-456 Mon.Google Scholar
Doazan, V., Franco, M., Rusconi, L., Sedmak, G. & Stalio, R. (1983). Astron. Astrophys. 128, 171.Google Scholar
Doazan, V., Grady, C.A., Snow, T.P., Peters, G.J., Marlborough, J.M., Barker, P.K., Bolton, C.T., Bourdonneau, B., Kuhi, L.V., Lyons, R.W., Polidan, R.S., Stalio, R. & Thomas, R.N. (1985). Astron. Astrophys. 152, 182.Google Scholar
Duschl, W.J. (1985). Unpublished Thesis, Univ. Munich.Google Scholar
Gies, D.R. & Bolton, C.T. (1986). Astrophys. J. 304, 371.Google Scholar
Gosset, E., Surdej, J. & Swings, J.-P. (1984). Astron.Astrophys.Suppl. 55, 411.Google Scholar
Gosset, E., Husemekers, D., Surdej, J. & Swings, J.-P. (1985). preprint.Google Scholar
Hall, D.S. (1981). In Solar Phenomena In Stars and Stellar Systems, ed. Bonnet, R.M. & Dupree, A.K., p.431. Dordrecht: D. Reidel.CrossRefGoogle Scholar
Harmanec, P. (1981). In Workshop on Pulsating B Stars, ed. G.E.V.O.N. & C. Sterken, p.99. Nice: Nice Obs. Publ. Google Scholar
Harmanec, P. (1982). IAU Symp. 98, 413.Google Scholar
Harmanec, P. (1983). In Workshop on Rapid Variability of Early-Type Stars, ed. Harmanec, P., & Pavlovski, K.. Hvar Obs. Bull. 7, 55.Google Scholar
Harmanec, P. (1984a). Bull.Astron.Inst.Czechosl. 35, 164.Google Scholar
Harmanec, P. (1984b). Bull.Astron.Inst.Czechosl. 35, 193.Google Scholar
Harmanec, P. (1984c). Inf.Bull.Var.Stars 2506.Google Scholar
Harmanec, P. (1985). Bull.Astron.Inst.Czechosl. 36, 327.Google Scholar
Harmanec, P. (1986). Inf.Bull.Var.Stars 2859.Google Scholar
Harmanec, P. & Kříž, S. (1976). IAU Symp. 70, 385.Google Scholar
Hensler, G. (1985). Astron.Astrophys. 148, 423.Google Scholar
Hubený, I., Štefl, S. & Harmanec, P. (1985). Bull.Astron.Inst.Czechosl. 16, 214.Google Scholar
Hubený, I., Harmanec, P. & Štefl, S. (1986). Bull.Astron.Inst.Czechosl. 37, No. 6.Google Scholar
Hudec, R. & Wenzel, W. (1976). Bull.Astron.Inst.Czechosl. 27, 325.Google Scholar
Huenemoerder, D.P. (1985). Astron.J. 90, 499.Google Scholar
Hutchings, J.B. & Hill, G. (1971). Astrophys.J. 167, 137.Google Scholar
Kippenhahn, R., Meyer-Hoffmeister, E. & Thomas, H.-C. (1970). Astron. Astrophys. 5, 155.Google Scholar
Kogure, T. (1984). In Proc. of Workshop on Stellar Activity and Observational Techiques Sino-Japan, Ed. J.-Y., Hu & Y.-S., Dong, p.l. Beijing: Beijing Obs., Acad. Sinica.Google Scholar
Kolka, I. (1983). Estonian Acad.Sci.Publ. (Phys.-Mat.) 32, 51.Google Scholar
Koubský, P., Horn, J., Harmanec, P., Peters, G.J., Polidan, R.S. & Barker, P.K. (1986). These Proceedings.Google Scholar
Kříž, S. (1979). Bull.Astron.Inst.Czechosl. 30, 83 & 95.Google Scholar
Kříž, S. & Harmanec, P. (1975). Bull.Astron.Inst.Czechosl. 26, 65.Google Scholar
Lucy, L.B. & Ricco, E. (1984). Astron.J. 84, 401.Google Scholar
Marlborough, J.M. (1982). IAU Symp. 98, 361.Google Scholar
Matese, J.J. & Whitmire, D.P. (1983). Astron.Astrophys. 117, L7.Google Scholar
Moulding, M. (1977). Astron.Astrophys. 58, 393.Google Scholar
Osaki, Y. (1986). Publ.Astron.Soc. Pacific 98, 30.Google Scholar
Penrod, G.D. (1986), Publ.Astron.Soc. Pacific 98, 35.CrossRefGoogle Scholar
Percy, J.R. (1979). Inf.Bull.Var. Stars 1530.Google Scholar
Percy, J.R. & Lane, M.C. (1979). Astron.J. 82, 353.Google Scholar
Percy, J.R., Jakate, S.M. & Matthews, J.M. (1981). Astron.J. 86, 53.Google Scholar
Plavec, M. (1976). IAU Symp. 70. 439.Google Scholar
Plavec, M.J. & Koch, R.H. (1978). Inf.Bull.Var. Stars 1482.Google Scholar
Plavec, M.J., Welland, J.L. & Koch, R.H. (1982). Astrophys.J. 256, 206.CrossRefGoogle Scholar
Pustylnik, I.B. & Einasto, L. (1984). Astrophys.Spa.Sci. 105, 259.CrossRefGoogle Scholar
Schuerman, D.W. (1972). Astrophys.Spa.Sci. 19, 351.Google Scholar
Slettebak, A. (1982). Astrophys.J.Suppl. 50, 55.Google Scholar
Slettebak, A. (1985). Astrophys.J.Suppl. 59, 769.Google Scholar
Smith, M.A. (1977). Astrophys.J. 215, 574.Google Scholar
Smith, M.A. (1978). Astrophys.J. 224, 927.Google Scholar
Smith, M.A. (1985). Astrophys.J. 297, 206 & 224.Google Scholar
Spear, G.G., Mills, J. Jr. & Snedden, S.A. (1981). Publ.Astron.Soc. Pacific 93, 460.CrossRefGoogle Scholar
Stagg, C.T., Božić, H., Fullerton, A., Gao, W.S., Guo, Z.H., Harmanec, P., Horn, J., Huang, L., Koubský, P., Pavlovski, K., Percy, J.R., Schmidt, F. & Štefl, S. (1985). J.Roy.Astron.Soc. Pacific 79, 243.Google Scholar
Štefl, S. (1986). These Proceedings.Google Scholar
Sterne, T.E. (1941). Proc.Nat.Acad.Sci.Amer. 27, 168.Google Scholar
Struve, O. (1944). Astrophys.J. 99, 89.Google Scholar
van Gent, R.H. & Lamers, H.J.G.L.M. (1986). Astron.Astrophys. 158, 335.Google Scholar
van't Veer, F. (1986). Astron.Astrophys. 156, 181.Google Scholar
Vogt, S.S. (1983). Astron.Astrophys. 118, 95.Google Scholar
Vogt, S.S. & Penrod, G.D. (1983). Astrophys.J. 275, 661.Google Scholar
Walker, M.F. (1953). Astrophys.J. 118, 481.Google Scholar
Walker, G.A.H., Yang, S. & Fahlman, S.S. (1979). Astrophys.J. 233, 199.Google Scholar
Walker, G.A.H., Yang, S. & Fahlman, S.S. (1981) In Workshop on Pulsating B Stars, ed. G.E.V.O.N., & Sterken, C., p.261. Nice: Nice Obs. Google Scholar