86 citations · 299 across the 7 of their papers we have counts for
7 papers
The nebular emission of star-forming galaxies in a hierarchical universe
Alvaro Orsi, Nelson Padilla, Brent Groves +4
Galaxy surveys targeting emission lines are characterising the evolution of star-forming galaxies, but there is still little theoretical progress in modelling their physical proper…
Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF
I. D. Gargiulo, S. A. Cora, N. D. Padilla +6
We make use of a semi-analytical model of galaxy formation to investigate the origin of the observed correlation between [a/Fe] abundance ratios and stellar mass in elliptical gala…
Calibration of semi-analytic models of galaxy formation using Particle Swarm Optimization
Andrés N. Ruiz, Sofía A. Cora, Nelson D. Padilla +8
We present a fast and accurate method to select an optimal set of parameters in semi-analytic models of galaxy formation and evolution (SAMs). Our approach compares the results of…
Chemical effects on the development of the colour-magnitude relation of cluster galaxies
Noelia Jiménez, Sofía A. Cora, Lilia P. Bassino +2
We investigate the development of the colour-magnitude re- lation (CMR) of cluster galaxies. This study is carried out using a semi- analytic model of galaxy formation and evolutio…
Ram pressure profiles in galaxy groups and clusters
Tomás E. Tecce, Sofía A. Cora, Patricia B. Tissera
Using a hybrid method which combines non-radiative hydrodynamical simulations with a semi-analytic model of galaxy formation, we determine the ram pressure as a function of halocen…
Ram pressure stripping in a galaxy formation model. I. A novel numerical approach
Tomás E. Tecce, Sofía A. Cora, Patricia B. Tissera +2
We develop a new numerical approach to describe the action of ram pressure stripping (RPS) within a semi-analytic model of galaxy formation and evolution which works in combination…
Analysis of the chemical evolution of the Galactic disk via dynamical simulations of the open cluster system
T. E. Tecce, L. J. Pellizza, A. E. Piatti
For several decades now, open clusters have been used to study the structure and chemical evolution of the disk of our Galaxy. Due to the fact that their ages and metallicities can…