activity
20042022
most citedThe O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and Te-based literature data

589 citations · 1.3k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.GA2022★ 41 cited

Mass-Metallicity and Star Formation Rate in Galaxies: a complex relation tuned to stellar age

S. Duarte Puertas, J. M. Vilchez, J. Iglesias-Páramo +5

In this work we study the stellar mass -- metallicity relation (MZR) of an extended sample of star-forming galaxies in the local Universe and its possible dependence with the star…

astro-ph.GA2021★ 11 cited

Aperture-corrected spectroscopic type Ia supernova host galaxy properties

Lluís Galbany, Mat Smith, Salvador Duarte Puertas +7

We use type Ia supernovae (SNe Ia) data obtained by the Sloan Digital Sky Survey-II Supernova Survey (SDSS-II/SNe) in combination with the publicly available SDSS DR16 fiber spectr…

astro-ph.GA2021★ 2 cited

A new insight of AGC198691 (Leoncino) galaxy with MEGARA at the GTC

E. Carrasco, M. L. García-Vargas, A. Gil de Paz +9

We describe the observations of the low-metallicity nearby galaxy AGC198691 (Leoncino dwarf) obtained with the Integral Field Unit of the instrument MEGARA at the Gran Telescopio C…

astro-ph.GA2021★ 3 cited

Impact of the external radiation field on the structure and evolution of supernova remnants

Mario Romero, Yago Ascasibar, Jan Palouš +2

We carry out 1D hydrodynamical simulations of the evolution of a spherically symmetric supernova remnant (SNR) subject to an external radiation field (ERF) that influences the cool…

astro-ph.GA2019★ 1 cited

The formation of the Galactic bulge in an inside-out scenario

O. Cavichia, M. Mollá

Chemical evolution models (CEM) are important tools to understand the formation and evolution of the components of the Milky Way Galaxy and other galaxies in the universe. The Gala…

astro-ph.GA2018★ 33 cited

The time evolution of the Milky Way's oxygen abundance gradient

M. Mollá, Á. I. Díaz, O. Cavichia +5

We study the evolution of oxygen abundance radial gradients as a function of time for the Milky Way Galaxy obtained with our {\sc Mulchem} chemical evolution model. We review the r…