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Influence of a Close Companion on the Variability of a Mira-Type Star

Published online by Cambridge University Press:  12 April 2016

G. M. Rudnitskij
G. M. Rudnitskij*
Affiliation:
Sternberg Astronomical Institute, Moscow State University, 13, Universitetskij Prospekt, Moscow, 119899, Russia

Abstract

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The effects of a low-mass companion (a planet?) revolving around a red giant at a short distance (inside its circumstellar envelope) are discussed. Calculations are given for a conical shock wave, induced by the orbital motion of the companion. Consequences for the stellar spectrum and light curve are derived, and predictions for the evolution of such a system are made.

Type
Part 5. Theoretical Models of Classical Pulsating Stars
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 384 - 385
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Bedding, T.R., Zijlstra, A.A., Von der Luhe, O., Robertson, J.G., Marson, R.G., Barton, J.R., & Carter, B.S. 1997, MNRAS, 286, 957 CrossRefGoogle Scholar
Castelaz, M.W. & Luttermoser, D.G. 1997, AJ, 114, 1584 CrossRefGoogle Scholar
Chapman, J.M. & Rudnitskij, G.M. 1999, Publ. Astron. Soc. Australia, submittedGoogle Scholar
Derviz, T.E. & Savanov, I.S. 1978, Soviet Ast., 22, 206 Google Scholar
Esipov, V.F., Lekht, E.E., Pashchenko, M.L., & Rudnitskij, G.M. 2000, in these proceedings, p. 126CrossRefGoogle Scholar
Harpaz, A. & Soker, N. (éd.) 1995, Asymmetrical Planetary Nebulae, University of Haifa at Oranim Conference, Annals of the Israel Physical Society, Volume 11 (Bristol & Philadelphia: Inst. Phys. Publ.; Jerusalem: Israel Phys. Soc.)Google Scholar
Knapp, G.R., Bowers, P.F., Young, K., & Phillips, T.G. 1995, ApJ, 455, 293 CrossRefGoogle Scholar
Lattanzi, M.G., Munari, U., Whitelock, P., & Feast, M.W. 1997, ApJ, 485, 328 CrossRefGoogle Scholar
López, B., Danchi, W.C., Bester, M., Hale, D.D.S., Lipman, E.A., Monnier, J.D., Tuthill, P.G., Townes, C.H., Degiacomi, C.G., Geballe, T.R., Greenhill, L.J., Cruzalèbes, P., Lefèvre, J., Mékarnia, D., Mattei, J.A., Nishimoto, D., & Kervin, P.W. 1997, ApJ, 488, 807 CrossRefGoogle Scholar
Reid, M.J. & Menten, K.M. 1997, ApJ, 476, 327 CrossRefGoogle Scholar
Soker, N. 1999, MNRAS, 306, 806 CrossRefGoogle Scholar
Struck-Marcell, C. 1988, ApJ, 330, 986 CrossRefGoogle Scholar
Udry, S., Jorissen, A., Mayor, M., & Van Eck, S. 1998, A&AS, 131, 25 Google Scholar