We present stellar parameters and metallicities for a sample of 64 high metal content stars not known to harbor any planet. This sample provides the reference for investigating new correlations between stars and the existence of an orbiting planet. © 2008 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Sousa, S. G., Santos, N. C., Israelian, G., Mayor, M., & Monteiro, M. J. P. F. G. (2008). Spectroscopic parameters for a sample of metal-rich solar-type stars. In ESO Astrophysics Symposia (Vol. 2008, pp. 319–320). https://doi.org/10.1007/978-3-540-75485-5_83
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