activity
20072026
most citedPopStar I: Evolutionary synthesis models description

154 citations · 200 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

MEGARA Stellar Spectral Library. Second Release

E. Carrasco, M. Lira-Franco, M. L. García-Vargas +6

We present the second release of the MEGARA spectral library, MEGASTAR, which now includes all spectra collected during ten observing semesters at the Gran Telescopio CANARIAS. Thi…

astro-ph.GA2023

Chemical evolution models: the role of type Ia supernovae in the -elements over Iron relative abundances and their variations in time and space

O. Cavichia, M. Mollá, J. J. Bazán +6

The role of type Ia supernovae (SN Ia), mainly the Delay Time Distributions (DTDs) determined by the binary systems, and the yields of elements created by different explosion mecha…

astro-ph.GA2023★ 4 cited

The multi-zone chemical evolution of the Galactic bulge: predicting abundances for different radial zones

Oscar Cavichia, Mercedes Mollá, Juanjo J. Bazán

Due to its proximity, the stellar populations of the Galactic bulge (GB) can be resolved and can be studied in detail. This allows tracing the bulge metallicity distribution functi…

astro-ph.SR2022★ 1 cited

MEGASTAR (III). Stellar parameters and data products for DR1 late-type stars

M. Mollá, M. L. García-Vargas, I. Millán-Irigoyen +5

MEGARA is the optical integral field and multi-object spectrograph at the Gran Telescopio Canarias. We have created MEGASTAR, an empirical library of stellar spectra obtained using…

astro-ph.GA2022★ 6 cited

Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories

I. Millan-Irigoyen, M. G. del Valle-Espinosa, R. Fernández-Aranda +5

We present a summary of our project that studies galaxies hosting type Ia supernova (SN Ia) at different redshifts. We present Gran Telescopio de Canarias (GTC) optical spectroscop…

astro-ph.GA2022★ 2 cited

Predicting interstellar radiation fields from chemical evolution models

Mario Romero, Pablo Corcho-Caballero, Iker Millán-Irigoyen +2

We present a self-consistent prediction of the interstellar radiation field (ISRF), from the extreme ultraviolet (EUV) to sub-mm range, based on two chemical evolution models of a…

astro-ph.SR2020★ 10 cited

MEGARA-GTC Stellar Spectral Library (I)

M. L. García-Vargas, E. Carrasco, M. Mollá +11

MEGARA (Multi Espectr{ó}grafo en GTC de Alta Resoluci{ó}n para Astronom{\'ı}a) is an optical (3650~--~9750Å), fibre-fed, medium-high spectral resolution (R = 6000, 12000, 20000) in…

astro-ph.GA2019★ 23 cited

2D-Galactic chemical evolution: the role of the spiral density wave

Mercedes Mollá, Sheillah Wekesa, Oscar Cavichia +6

We present a 2-dimensional chemical evolution code applied to a Milky Way type galaxy, incorporating the role of spiral arms in shaping azimuthal abundance variations, and confront…

astro-ph.GA2016

Galactic Chemical Evolution

M. Mollá, O. Cavichia, R. da Costa +2

We analyze the evolution of oxygen abundance radial gradients resulting from our chemical evolution models calculated with different prescriptions for the star formation rate (SFR)…

astro-ph.CO2009★ 154 cited

PopStar I: Evolutionary synthesis models description

M. Molla, M. L. Garcia-Vargas, A. Bressan

We present new evolutionary synthesis models for Simple Stellar Populations for a wide range of ages and metallicities. The models are based on the Padova isochrones. The core of t…

astro-ph2007

The H density within spiral and irregular galaxies at high redshift: estimating CO detection limits

Mercedes Mollá, Eduardo Hardy, '{A}ngeles I. Díaz

We have computed a grid of chemical evolution models for a large set of spiral and irregular theoretical galaxies of different total mass. In our models, the gas phase has two comp…