Abundances of Volatiles C, N and S in Stars with Exoplanets
Not Available
Ecuvillon, A. et al.
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2004
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Abundances in Stars with ExoplanetsExtensive spectroscopic studies of stars with and without planets have concluded that stars hosting planets are significantly more metal-rich than those without planets. More subtle trends of different chemical elements begin to appear as the number of detected extrasolar planetary systems continues to grow. I review our current knowledgeIsraelian, G.
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A Correlation between Light Profile and [Mg/Fe] Abundance Ratio in Early-Type GalaxiesWe explore possible correlations between light profile shapes, as parameterized by the Sérsic index n or the concentration index Cre(1/3), and relevant stellar population parameters in early-type galaxies. Mean luminosity-weighted ages, metallicities, and abundance ratios were obtained from spectra of very high signal-to-noise ratio and stellarVazdekis, Alexandre et al.
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XRF 040916, optical follow-up.Not Availablede Ugarte Postigo, A. et al.
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XRF 040912, identification of CXO sources.Not AvailableGorosabel, J. et al.
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XMM-newton images of GRB 040827.Not AvailableRodriguez-Pascual, P. et al.
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02004