Photospheric and coronal abundances in solar-type stars: the peculiar case of Tau Bootis

Abstract

Chemical abundances in solar-type stars are a much debated topic. Planet-hosting stars are known to be metal-rich, but whether or not this peculiarity applies also to the chemical composition of the outer stellar atmospheres is still to be clarified. More in general, coronal and photospheric abundances in late-type stars appear to be different in many cases, but understanding how chemical stratification effects work in stellar atmospheres requires an observational base larger than currently available. We obtained XMM-Newton high-resolution X-ray spectra of Tau Bootis, a well known nearby star with a Jovian-mass close-in planet. We analyzed these data with the aim to perform a detailed line-based emission measure analysis and derive the abundances of individual elements in the corona with two different methods applied independently. We compared the coronal abundances of Tau Bootis with published photospheric abundances based on high-resolution optical spectra and with those of other late-type stars with different magnetic activity levels, including the Sun. We find that the two methods provide consistent results within the statistical uncertainties for both the emission measure distribution of the hot plasma and for the coronal abundances, with discrepancies at the 2-sigma level limited to the amount of plasma at temperatures of 3-4 MK and to the O and Ni abundances. In both cases, the elements for which both coronal and photospheric measurements are available (C, N, O, Si, Fe, and Ni) result systematically less abundant in the corona by a factor 3 or more, with the exception of the coronal Ni abundance, which is similar to the photospheric value. Comparison with other late-type stars of similar activity level shows that these coronal/photospheric abundance ratios are peculiar to Tau Bootis and possibly related to the characteristic over-metallicity of this planet-hosting star.

9 pages, 7 figures. A&A, in press. Language-edited version, one reference updated

References in corpus (11)

• Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog
• The On/Off Nature of Star-Planet Interactions
• X-Ray Spectroscopy of Stars
• Magnetic cycles of the planet-hosting star tauBootis
• CHARA Array Measurements of the Angular Diameters of Exoplanet Host Stars
• The magnetic field of the planet-hosting star $\tau$ Bootis
• MOST detects variability on tau Bootis possibly induced by its planetary companion
• A scenario of planet erosion by coronal radiation
• The Chemical Compositions of Stars with Planets: A Review
• Parent Stars of Extrasolar Planets. VIII. Chemical Abundances for 18 Elements in 31 Stars
• Neon and oxygen in low activity stars: towards a coronal unification with the Sun

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• The FIP and Inverse FIP Effects in Solar and Stellar Coronae
• The stellar wind cycles and planetary radio emission of the Tau Boo system
• A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: Hipparcos-Tycho cool stars
• A coordinated optical and X-ray spectroscopic campaign on HD179949: searching for planet-induced chromospheric and coronal activity
• A Chandra/LETGS Survey of Main Sequence Stars
• Connection between planetary He I $\lambda$10830 Å absorption and extreme-ultraviolet emission of planet-host stars
• The Coronal Abundances of Mid-F Dwarfs
• A magnetic cycle of tau Bootis? The coronal and chromospheric view
• Space environment and magnetospheric Poynting fluxes of the exoplanet $\tau$ Boötis b
• Coronae of Stars with Super Solar Elemental Abundances
• Chandra Characterization of X-ray Emission in the Young F-Star Binary System HD 113766
• Stellar Coronal and Wind Models: Impact on Exoplanets