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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S265(5), p. 436-437, 2009

DOI: 10.1017/s1743921310001201

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Photospheric and coronal abundances of solar-type stars with planets: the case of τ Bootis

Journal article published in 2009 by Antonio Maggio ORCID, Jorge Sanz-Forcada ORCID, Luigi Scelsi
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractWe present the results of a study of coronal and photospheric abundances in τ Bootis, a middle-aged solar analogue, well known for the presence of a close-in Jovian mass planet. We employ the results of this study, based on high-resolution optical and X-ray spectra, to address the issue of abundance stratification vs. First Ionization Potential (FIP) in the outer stellar atmospheres of solar-type stars with and without planets.

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