activity
20112021
most citedOn the galaxy spiral arms' nature as revealed by rotation frequencies

80 citations · 147 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2021★ 2 cited

Nauyaca: a new tool to determine planetary masses and orbital elements through transit timing analysis

Eliab F. Canul, Héctor Velázquez, Yilen Gómez Maqueo Chew

Transit Timing Variations (TTVs) is currently the most successful method to determine dynamical masses and orbital elements for Earth-sized transiting planets. Precise mass determi…

astro-ph.CO2020

Assessing the Hierarchical Hamiltonian Splitting Integrator for Collisionless N-body Simulations

G. Aguilar-Argüello, O. Valenzuela, J. C. Clemente +2

The large dynamic range in some astrophysical N-body problems led to the use of adaptive multi-time-steps; however, the search for optimal strategies is still challenging. We numer…

astro-ph.GA2015★ 26 cited

GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons

Santi Roca-Fàbrega, Octavio Valenzuela, Pedro Colín +5

We introduce a new set of simulations of Milky Way-sized galaxies using the AMR code ART + hydrodynamics in a CDM cosmogony. The simulation series is named GARROTXA and follow t…

astro-ph.GA2013★ 80 cited

On the galaxy spiral arms' nature as revealed by rotation frequencies

Santi Roca-Fàbrega, Octavio Valenzuela, Francesca Figueras +4

High resolution N-body simulations using different codes and initial condition techniques reveal two different behaviours for the rotation frequency of transient spiral arms like s…

astro-ph.CO2011★ 39 cited

The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations

V. Avila-Reese, P. Colín, A. González-Samaniego +4

(Abridged) By means of high-resolution cosmological simulations in the context of the LCDM scenario, the specific star formation rate (SSFR=SFR/Ms, Ms is the stellar mass)--Ms and…