96 citations · 129 across the 2 of their papers we have counts for
5 papers
The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
Enrique Vázquez-Semadeni, Aina Palau, Gilberto C. Gómez +8
We provide a detailed comparison between the ``turbulent support'' (TS) and ``global hierarchical collapse'' (GHC) models for molecular clouds and star formation, their respective…
The effect of photoionising feedback on the shaping of hierarchically-forming stellar clusters
Alejandro González-Samaniego, Enrique Vazquez-Semadeni
We use two hydrodynamical simulations (with and without photoionising feedback) of the self-consistent evolution of molecular clouds (MCs) undergoing global hierarchical collapse (…
Optical Integral Field Spectroscopy observations applied to simulated galaxies: Testing the fossil record method
Héctor J. Ibarra-Medel, Vladimir Avila-Reese, Sebastián F. Sánchez +2
By means of post-processed cosmological Hydrodynamics simulations we explore the ability of the fossil record method to recover the stellar mass, age gradients, and global/radial s…
SIDM on FIRE: Hydrodynamical Self-Interacting Dark Matter simulations of low-mass dwarf galaxies
Victor H. Robles, James S. Bullock, Oliver D. Elbert +7
We compare a suite of four simulated dwarf galaxies formed in 10 haloes of collisionless Cold Dark Matter (CDM) with galaxies simulated in the same haloes with an…
Dwarf Galaxy Mass Estimators vs. Cosmological Simulations
Alejandro Gonzalez-Samaniego, James S. Bullock, Michael Boylan-Kolchin +5
We use a suite of high-resolution cosmological dwarf galaxy simulations to test the accuracy of commonly-used mass estimators from Walker et al.(2009) and Wolf et al.(2010), both o…