activity
19982021
most citedThe Nitrogen-to-Oxygen evolution in galaxies: the role of the star formation rate

104 citations · 502 across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2021★ 20 cited

HR-pyPopStar: high wavelength-resolution stellar populations evolutionary synthesis model

I. Millán-Irigoyen, M. Mollá, M. Cerviño +3

We present the HR-pyPopStar model, which provides a complete set (in ages) of high resolution (HR) Spectral Energy Distributions of Single Stellar Populations. The model uses the m…

astro-ph.GA2019★ 64 cited

SIGNALS: I. Survey Description

L. Rousseau-Nepton, R. P. Martin, C. Robert +60

SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing program designed to investigate massive star formation and HII regions in a sam…

astro-ph.GA2016★ 1 cited

The evolution of the Oxygen abundance radial gradient in the Milky Way Galaxy disk

M. Mollá, O. Cavichia, R. D. D Costa +3

We review the state of our chemical evolution models for spiral and low mass galaxies. We analyze the consequences of using different stellar yields, infall rate laws and star form…

astro-ph.GA2016

Properties of the outer regions of spiral disks: abundances, colors and ages

Mercedes Mollá, Angeles I. Díaz, Brad K. Gibson +2

We summarize the results obtained from our suite of chemical evolution models for spiral disks, computed for different total masses and star formation efficiencies. Once the gas, s…

astro-ph.CO2012★ 63 cited

A two-phase scenario for bulge assembly in LCDM cosmologies

A. Obreja, R. Domínguez-Tenreiro, C. Brook +5

We analyze and compare the bulges of a sample of L* spiral galaxies in hydrodynamical simulations in a cosmological context, using two different codes, P-DEVA and GASOLINE. The cod…

astro-ph.GA2010

Some caveats about the evolution of the N/O abundance and the star formation history

M. Molla, M. Gavilan

We carefully analyze how the abundance of Nitrogen over Oxygen evolves when dependent on metallicity stellar yields with a primary component of N proceeding from AGBs stars are use…