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The long secondary periods in semi-regular variables

  • P.R. Wood (a1), A.E. Olivier (a1) and S.D. Kawaler (a2)
Abstract

About 25% of variable asymptotic giant branch stars in the LMC have light curves that are modulated by a long secondary period of length ~ 1–4 yr. Solar-vicinity analogs of these stars show radial velocity curves that are asymmetric and of small amplitude (~3–5km s−1). Possible explanations for the photometric and radial velocity variations include: eccentric motion of an orbiting companion of mass ~0.1 M; radial and nonradial pulsation; rotation of an ellipsoidal-shaped red giant; episodic dust ejection; and star spot cycles. We find that there are severe difficulties with each of these models. Thus, the long secondary periods are the only unexplained type of large-amplitude stellar variability known at this time.

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References
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Hinkle, K.H., Lebzelter, T., Joyce, R.R., Fekel, F.C. 2002, AJ, 123, 1002
Höfner, S., Feuchtinger, M.U., Dorfi, E.A. 1995, A&A, 297, 815
Houk, N. 1963, AJ, 68, 253
Kiss, L.L., Szatmáry, K., Cadmus, R.R. Jr, Mattei, J.A. 1999, A&A, 346, 542
Luttermoser, D.G., Johnson, H.R. Eaton, J. 1994, ApJ, 422, 351
Olivier, E.A., Wood, P.R. 2003, ApJ, 584, 1035
Payne-Gaposhkin, C. 1954, Harvard Annals, 113, No. 4
Percy, J.R., Bakos, G.A. 2003, preprint
Winters, J.M., Fleischer, A.J., Gauger, A., Sedlmayr, E. 1994, A&A, 290, 623
Wood, P.R. and the MACHO COLLABORATION 1999, in IAU Symposium 191, AGB Stars, eds. Le Bertre, T., Lèbre, A. & Waelkens, C. (San Francisco, ASP), 151
Wood, P.R. 2000, in IAU Coll. 176, ASP Conf. Ser. Vol. 203, The Impact of Large-Scale Surveys on Pulsating Star Research, eds Szabados, L. & Kurtz, D. (San Francisco, ASP), 379
Wood, P.R., Olivier, E.A., Kawaler, S. 2003, ApJ, submitted
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0252-9211
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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