Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-28T22:32:12.396Z Has data issue: false hasContentIssue false
  • English
  • Français

Glimpses of Be Binary Evolution

Published online by Cambridge University Press:  12 April 2016

Douglas R. Gies
Douglas R. Gies*
Affiliation:
Center for High Angular Resolution Astronomy, Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30303, U.S.A

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.

Models of close binary evolution predict that mass gainers will be spun up to speeds close to the critical rotational velocity while the mass donors will appear as stripped down He stars, white dwarfs, or neutron stars. I argue here that the mass gainers are closely related to the Be stars. I present a list of the known Be binary systems which consists of those with bright, Roche-filling companions and those with faint or undetected companions. Notably absent are Be + B systems which are expected if the Be phase is a stage in the life of a single star. We now have the first example of a Be + He star system in the binary, ϕ Per, and taken together with the well known Be X-ray binaries, there is clear evidence that some fraction of Be stars are created in binaries; whether all such rapid rotators are so formed remains unknown.

Type
7. Interacting Binaries
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 668 - 680
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Abt, H.A., & Cardona, O. 1984, ApJ, 285, 190 CrossRefGoogle Scholar
Abt, H.A., & Levy, S.G. 1978, ApJS, 36, 241 [Abt 1978]CrossRefGoogle Scholar
Anderson, J., Pavlovski, K., & Piirola, V. 1989, A&A, 215, 272 Google Scholar
Baade, D. 1992, in Evolutionary Processes in Interacting Binary Stars, ed. Kondo, Y., Sistero, R., & Polidan, R.S. (Dordrecht: Kluwer Academic), 147 CrossRefGoogle Scholar
Bagnuolo, W.G. Jr., Gies, D.R., Hahula, M.E., Wiemker, R., & Wiggs, M.S. 1994, ApJ, 423, 446 CrossRefGoogle Scholar
Balachandran, S., Lambert, D.L., Tomkin, J., & Parthasarathy, M. 1986, MNRAS, 219, 479 CrossRefGoogle Scholar
Batten, A.H., Fletcher, J.M., & MacCarthy, D.G. 1989, Publ. DAO, 17 Google Scholar
Bolton, C.T., Harmanec, P., Lyons, R.W., Odell, A.P., & Pyper, D.M. 1998, A&A, 337, 183 Google Scholar
Bossi, M., Nunez, N.S., Guerrero, G., Sareyan, J.-P., & Alvarez, M. 1998, A&AS, 127, 433 Google Scholar
Budding, E. 1984, CDS Bull., 27, 91 Google Scholar
Burleigh, M.R., & Barstow, M.A. 1999, A&A, 341, 795 Google Scholar
De Loore, C.W.H., & Doom, C. 1992, Structure and evolution of single and binary stars (Dordrecht: Kluwer Academic)CrossRefGoogle Scholar
De Loore, C., & Vanbeveren, D. 1995, A&A, 304, 220 Google Scholar
Dempsey, R.C., Parsons, S.B., Bopp, B.W., & Fekel, F.C. 1990, PASP, 102, 312 [Deml990]CrossRefGoogle Scholar
Dudley, R.E., & Jeffery, C.S. 1990, MNRAS, 247, 400 Google Scholar
Duemmler, R., Kubicela, A., Doazan, V., Bourdonneau, B., & Arsenijevic, J. 1988, A&AS, 75, 311 [Duel988]Google Scholar
Eggen, O.J. 1983, AJ, 88, 1676 CrossRefGoogle Scholar
Elias, N.M. II, Wilson, R.E., Olson, E.C., Aufdenberg, J.P., Guinan, E.F., Guedel, M., van Hamme, W.V., & Stevens, H.L. 1997, ApJ, 484, 394 [Eli11997]CrossRefGoogle Scholar
Etzel, P.B. 1988, AJ, 95, 1204 CrossRefGoogle Scholar
Etzel, P.B., & Olson, E.C. 1993, AJ, 106, 1200 CrossRefGoogle Scholar
Fabregat, J., & Torrejón, J.M. 2000, A&A, 357, 451 Google Scholar
Floquet, M., Hubert, A.M., Chauville, J., Chatzichristou, H., & Maillard, J.-P. 1989, A&A, 214, 295 Google Scholar
Floquet, M., Hubert, A.M., Hubert, H., Ballereau, D., & Chauville, J. 1995, A&A, 294, 227 Google Scholar
Gies, D.R., Bagnuolo, W.G. Jr., Ferrara, E.C., Kaye, A.B., Thaller, M.L., Penny, L.R., & Peters, G.J. 1998, ApJ, 493, 440 [Giel998]CrossRefGoogle Scholar
Griffin, R.F., Parsons, S.B., Dempsey, R., & Bopp, B.W. 1990, PASP, 102, 535 [Gri1990]CrossRefGoogle Scholar
Habets, G.M.J.H. 1986, A&A, 167, 91 Google Scholar
Harmanec, P. 1984, Bull. Astr. Inst. Cz., 35, 164 [Harl984]Google Scholar
Harmanec, P. 1987a, in Physics of Be Stars, ed. Slettebak, A. & Snow, T.P.(Cambridge: Cambridge Univ.), 339 Google Scholar
Harmanec, P. 1987b, Bull. Astr. Inst. Cz., 38, 283 [Harl987]Google Scholar
Harmanec, P., Koubský, P., & Krpata, J. 1974, A&A, 33, 117 Google Scholar
Harmanec, P., & Křiž, S. 1976, in Be and Shell Stars, ed. Slettebak, A. (Dordrecht: Reidel), 385 CrossRefGoogle Scholar
Harmanec, P., et al. 1996, A&A, 312, 879 Google Scholar
Hendry, E.M., & Bahng, J.D.R. 1981, J. Ap&A, 2, 141 Google Scholar
Hill, G., Harmanec, P., Pavlovski, K., Božić, H., Hadrava, P., Koubský, P., & Ziznovsky, J. 1997, A&A, 324, 965 [Hil11997]Google Scholar
Hill, S.N. 1929, Publ. DAO, 4, 261 [Hil1929]Google Scholar
Hubert, A.M., et al. 1997, A&A, 324, 929 Google Scholar
Jarad, M.M., Hilditch, R.W., & Skillen, I. 1989, MNRAS, 238, 1085 [Jarl989]CrossRefGoogle Scholar
Juza, K., Harmanec, P., Hill, G., Tarasov, A.E., Matthews, J.M., Tuominen, I., & Yang, S. 1991, Bull. Astr. Inst. Cz., 42, 39 [Juzl991]Google Scholar
Kaitchuck, R.H., Honeycutt, B.K., & Schlegel, E.M. 1985, PASP, 97, 1178 CrossRefGoogle Scholar
Katahira, J., Hirata, R., Ito, M., Katoh, M., Ballereau, D., & Chauville, J. 1996, PASJ, 48, 317 [Katl996]CrossRefGoogle Scholar
Kogure, T., & Suzuki, M. 1986, Ap&SS, 127, 143 Google Scholar
Koubský, P., et al. 1989, Bull. Astr. Inst. Cz., 40, 31 [Koul989]Google Scholar
Koubský, P., et al. 1997, A&A, 328, 551 [Koul997]Google Scholar
Křiž, S., & Harmanec, P. 1975, Bull. Astr. Inst. Cz., 26, 65 Google Scholar
Lawson, W.A., Clark, M., & Cottrell, P.L. 1994, MNRAS, 266, 740 [Lawl994]CrossRefGoogle Scholar
Lipunov, V.M., Postnov, K.A., & Prokhorov, M.E. 1996, A&A, 310, 489 Google Scholar
Mason, B.D. 1997, AJ, 114, 808 CrossRefGoogle Scholar
Mason, B.D., ten Brummelaar, T., Gies, D.R., Hartkopf, W.I., & Thaller, M.L. 1997, AJ, 114, 2112 CrossRefGoogle Scholar
Mason, B.D., Gies, D.R., Hartkopf, W.I., Bagnuolo, W.G. Jr., ten Brummelaar, T., & McAlister, H.A. 1998, AJ, 115, 821 CrossRefGoogle Scholar
Matthews, J.M., Harmanec, P., Walker, G.A.H., Yang, S., & Wehlau, W.H. 1991, MNRAS, 248, 787 [Matl991]CrossRefGoogle Scholar
Meurs, E.J.A., et al. 1992, A&A, 265, L41 Google Scholar
Negueruela, I. 1998, A&A, 338, 505 Google Scholar
Olson, E.C., & Etzel, P.B. 1995, AJ, 109, 345 [Ols1995]CrossRefGoogle Scholar
Olson, E.C., & Plavec, M.J. 1997, AJ, 113, 425 [Ols1997]CrossRefGoogle Scholar
Olson, E.C., Schaefer, B., Lines, R., Lines, H., & Fried, R. 1992, AJ, 103, 256 CrossRefGoogle Scholar
Packet, W. 1981, A&A, 102, 17 Google Scholar
Parsons, S.B., & Bopp, B.W. 1993, BAAS, 25, 1376 [Par1993]Google Scholar
Peters, G.J. 1976, in Be and Shell Stars, ed. Slettebak, A. (Dordrecht: Reidel), 417 CrossRefGoogle Scholar
Peters, G.J. 1983, PASP, 95, 311 [Petl983]CrossRefGoogle Scholar
Peters, G.J. 1988, ApJ, 331, L33[Petl988]CrossRefGoogle Scholar
Peters, G.J. 1989, Space Sci. Rev., 50, 9 CrossRefGoogle Scholar
Peters, G.J. 1999, private communication [Petl999]Google Scholar
Peters, G.J., & Polidan, R.S. 1998, ApJ, 500, L17 CrossRefGoogle Scholar
Plavec, M. 1976, in Be and Shell Stars, ed. Slettebak, A. (Dordrecht: Reidel), 439 CrossRefGoogle Scholar
Poeckert, R. 1981, PASP, 93, 297 CrossRefGoogle Scholar
Polidan, R.S. 1976, in Be and Shell Stars, ed. Slettebak, A. (Dordrecht: Reidel), 401 CrossRefGoogle Scholar
Pols, O.R., Coté, J., Waters, L.B.F.M., & Heise, J. 1991, A&A, 241, 419 Google Scholar
Popper, D.M. 1989, ApJS, 71, 595 [Popl989]CrossRefGoogle Scholar
Portegies Zwart, S.F. 1995, A&A, 296, 691 Google Scholar
Quirrenbach, A., et al. 1997, ApJ, 479, 477 CrossRefGoogle Scholar
Rappaport, S.A., & van den Heuvel, E.P.J. 1982, in Be Stars, ed. Jaschek, M. & Groth, H.G. (Dordrecht: Reidel), 327 CrossRefGoogle Scholar
Richards, M.T., Koubský, P., Šimon, V., Peters, G.J., Hirata, R., Škoda, P., & Masuda, S. 2000, ApJ, 531, 100 [Ric2000]CrossRefGoogle Scholar
Richards, M.T., & Ratliff, M.A. 1998, ApJ, 493, 326 CrossRefGoogle Scholar
Rivinius, Th., 1999, private communication (see also Rivinius & Štefl, these proc, p.581) [Riv1999]CrossRefGoogle Scholar
Sahade, J., Ferrer, O., Garcia, L.G., Brandi, E., & Barba, R. 1997, PASP, 109, 1237 [Sahl997]CrossRefGoogle Scholar
Sanford, R.F. 1926, ApJ, 64, 172 [Sanl926]CrossRefGoogle Scholar
Slettebak, A. 1982, ApJS, 50, 55 CrossRefGoogle Scholar
Štefl, S., Harmanec, P., Horn, J., Koubský, P., Křiž, S., Hadrava, P., Božić, H., & Pavlovski, K. 1990, Bull. Astr. Inst. Cz., 41, 29 Google Scholar
Tarasov, A.E., Berdyugina, S.V., & Berdyugin, A.V. 1998, PAZh, 24, 375[Tarl998]Google Scholar
Tarasov, A.E., & Tuominen, I. 1987, Publ. Astr. Inst. Czechosl. Acad. Sci., 70 (lOth Euro. Reg. Astr. Meeting - IAU), ed. Harmanec, P., 127 Google Scholar
Thaller, M.L., Bagnuolo, W.G. Jr., Gies, D.R., & Penny, L.R. 1995, ApJ, 448, 878 CrossRefGoogle Scholar
Tur, N.S., Goraya, P.S., & Sharma, S.D. 1995, PASP, 107, 730 CrossRefGoogle Scholar
Van Bever, J., & Vanbeveren, D. 1997, A&A, 322, 116 Google Scholar
Vanbeveren, D., van Rensbergen, W., & De Loore, C. 1998, The Brightest Binaries (Dordrecht: Kluwer Academic)CrossRefGoogle Scholar
van der Linden, T.J. 1987, A&A, 178, 170 Google Scholar
Vennes, S., Berghöfer, T., & Christian, D. 1997, ApJ, 491, L85 CrossRefGoogle Scholar
Wang, Z., & Gies, D.R. 1998, PASP, 110, 1310 CrossRefGoogle Scholar
Waters, L.B.F.M., Coté, J., & Pols, O.R. 1991, A&A, 250, 437 Google Scholar
Waters, L.B.F.M., Pols, O.R., Hogeveen, S.J., Coté, J., & van den Heuvel, E.P.J. 1989, A&A, 220, L1 Google Scholar
Welty, A.D., & Wade, R.A. 1995, AJ, 109, 327 [Wel1995]Google Scholar
Wilson, R.E., & Plavec, M.J. 1988, AJ, 95, 1828 [Wil1988]CrossRefGoogle Scholar