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Seismic Constraint on the Plausible Explanations of the Metal Rich Feature of Planetary System Stars

  • H. Shibahashi (a1) and S. Watanabe (a1)

Abstract

From Spectroscopic observations showing that the parent stars of planetary systems are metal rich, it is suspected that this feature results from the accompanying planetary system. With the rich helioseismic data so far obtained, we determine the metal abundance distribution in the solar interior with respect to the distance from the center. This result gives constraints on the possible explanations about the metal rich feature of the stars accompanied by a planetary system.

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References

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Basu, S. 1998, MNRAS, 298, 719
Deubner, F.-L., et al. (eds.) 1998, New eyes to see inside the Sun and stars, (Kluwer Academic Publishers)
Gonzalez, G., Laws, C., Tyagi, S., & Reddy, B.E. 2001, AJ, 121, 432
Snow, T.P. & Witt, A.N. 1996, ApJ, 468, L65
Takata, M. & Shibahashi, H. 1998, ApJ, 504, 1035
Watanabe, S. & Shibahashi, H. 2001, PASJ, submitted

Seismic Constraint on the Plausible Explanations of the Metal Rich Feature of Planetary System Stars

  • H. Shibahashi (a1) and S. Watanabe (a1)

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