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20012019
most citedC, S, Zn and Cu abundances in planet-harbouring stars

112 citations · 254 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2019★ 39 cited

Clocking the assembly of double-barred galaxies with the MUSE TIMER project

A. de Lorenzo-Cáceres, P. Sánchez-Blázquez, J. Méndez-Abreu +11

The formation of two stellar bars within a galaxy has proved challenging for numerical studies. It is yet not clear whether the inner bar is born via a star formation process promo…

astro-ph.CO2009★ 26 cited

Search for blue compact dwarf galaxies during quiescence II: metallicities of gas and stars, ages, and star-formation rates

J. Sanchez Almeida, J. A. L. Aguerri, C. Munoz-Tunon +1

We examine the metallicity and age of a large set of SDSS/DR6 galaxies that may be Blue Compact Dwarf (BCD) galaxies during quiescence (QBCDs).The individual spectra are first clas…

astro-ph2008★ 47 cited

Search for Blue Compact Dwarf Galaxies During Quiescence

J. Sanchez Almeida, C. Munoz-Tunon, R. Amorin +3

Blue Compact Dwarf (BCD) galaxies are metal poor systems going through a major starburst that cannot last for long. We have identified galaxies which may be BCDs during quiescence…

astro-ph2005

Abundance ratios of volatile vs. refractory elements: hints of pollutions?

A. Ecuvillon, G. Israelian, N. C. Santos +2

We present the abundance ratios [X/H] of a large set of chemical species with condensation temperatures from 75 to 1600 K in an almost complete set of 105 planet-host stars and in…

astro-ph2004★ 112 cited

C, S, Zn and Cu abundances in planet-harbouring stars

A. Ecuvillon, G. Israelian, N. C. Santos +3

We present a detailed and uniform study of C, S, Zn and Cu abundances in a large set of planet host stars, as well as in a homogeneous comparison sample of solar-type dwarfs with n…

astro-ph2003★ 30 cited

The Line Emission Region in III Zw 2: Kinematics and Variability

L. C. Popovic, E. G. Mediavilla, E. Bon +2

We have studied the Ly-al, Hbeta, Halpha and Mg II2798 line profiles of the Seyfert 1 galaxy III Zw 2. The shapes of these broad emission lines show evidence of a multicomponent or…