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20012023
most citedSpectroscopic [Fe/H] for 98 extra-solar planet-host stars: Exploring the probability of planet formation

960 citations · 4.4k across the 30 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2017★ 2 cited

Abundance ratios \& ages of stellar populations in HARPS-GTO sample

E. Delgado Mena, M. Tsantaki, V. Zh. Adibekyan +4

In this work we present chemical abundances of heavy elements (Z28) for a homogeneous sample of 1059 stars from HARPS planet search program. We also derive ages using parallaxes…

astro-ph.SR2017★ 41 cited

SWEET-Cat update and FASMA. A new minimization procedure for stellar parameters using high-quality spectra

D. T. Andreasen, S. G. Sousa, M. Tsantaki +6

Context: Thanks to the importance that the star-planet relation has to our understanding of the planet formation process, the precise determination of stellar parameters for the ev…

astro-ph.SR2016★ 51 cited

CNO behaviour in planet-harbouring stars. II. Carbon abundances in stars with and without planets using the CH band

L. Suárez-Andrés, G. Israelian, J. I. González Hernández +4

Context. Carbon, oxygen and nitrogen (CNO) are key elements in stellar formation and evolution, and their abundances should also have a significant impact on planetary formation an…

astro-ph.SR2016★ 34 cited

Abundance trend with condensation temperature for stars with different Galactic birth places

V. Adibekyan, E. Delgado-Mena, P. Figueira +9

During the past decade, several studies reported a correlation between chemical abundances of stars and condensation temperature (also known as Tc trend). However, the real astroph…

astro-ph.SR2016★ 44 cited

Searching for Li-rich giants in a sample of 12 open clusters: Li enhancement in two stars with substellar companions

E. Delgado Mena, M. Tsantaki, S. G. Sousa +6

The aim of this work is to search for Li-rich giants in a sample of clusters where planets have been searched, thus we can study the planet engulfment scenario to explain Li replen…

astro-ph.SR2014★ 148 cited

Li abundances in F stars: planets, rotation and galactic evolution

E. Delgado Mena, S. Bertrán de Lis, V. Zh. Adibekyan +7

We find that hot jupiter host stars within the T range 5900-6300K show lower Li abundances, by 0.14 dex, than stars without detected planets. This offset has a signi…