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- W3100228679 abstract "Aims.This paper presents detailed analysis and modelisation of the star HD 17051 (alias ι Hor), which appears to be a specially interesting case among exoplanet host stars. Like most of these stars, ι Hor presents a metallicity excess that has been measured by various observers who give different results, ranging from [ Fe/H to 0.26 and associated with different atmospheric parameters. Meanwhile, the luminosity of the star may be determined thanks to the Hipparcos parallax. Although it is in the southern hemisphere, this star belongs to the Hyades stream, and its external parameters show that it could even be one of the Hyades stars ejected during cluster formation. The aim of this work was to gather and analyse our present knowledge of this star and to prepare seismic tests for future observations with the HARPS spectrometer (planned for November 2006)." @default.
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- W3100228679 date "2006-11-20" @default.
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- W3100228679 title "Asteroseismology of exoplanets host stars: the special case of ι Horologii (HD 17051)" @default.
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- W3100228679 doi "https://doi.org/10.1051/0004-6361:20066083" @default.
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