S
Stefano Bovino
Researcher at University of Concepción
Publications - 117
Citations - 2415
Stefano Bovino is an academic researcher from University of Concepción. The author has contributed to research in topics: Star formation & Stars. The author has an hindex of 25, co-authored 106 publications receiving 2000 citations. Previous affiliations of Stefano Bovino include Kavli Institute for Theoretical Physics & Sapienza University of Rome.
Papers
More filters
Journal ArticleDOI
KROME - a package to embed chemistry in astrophysical simulations
Tommaso Grassi,Stefano Bovino,Dominik R. G. Schleicher,Joaquin Prieto,Daniel Seifried,E. Simoncini,Franco A. Gianturco,Franco A. Gianturco +7 more
TL;DR: An extended test suite ranging from one-zone and 1D-models to first applications including cosmological simulations with ENZO and RAMSES and 3D collapse simulations with the FLASH code is presented.
Journal ArticleDOI
How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
Muhammad Latif,Stefano Bovino,Tommaso Grassi,Tommaso Grassi,Dominik R. G. Schleicher,Marco Spaans +5 more
TL;DR: In this paper, the authors derived the critical value of such a flux for realistic spectra of Pop II stars through three-dimensional cosmological simulations and derived the dependence of J21}^crit on the radiation spectra, on variations from halo to halo, and on the impact of X-ray ionization.
Journal ArticleDOI
The Turbulent Dynamo in Highly Compressible Supersonic Plasmas
TL;DR: In this paper, a quantitative comparison of theoretical models of the dynamo growth rate and saturation level with three-dimensional magnetohydrodynamical simulations of supersonic turbulence with grid resolutions of up to 1024{sup 3} cells was performed.
Journal ArticleDOI
A UV flux constraint on the formation of direct collapse black holes
Muhammad Latif,Stefano Bovino,C. Van Borm,Tommaso Grassi,Tommaso Grassi,Dominik R. G. Schleicher,Marco Spaans +6 more
TL;DR: In this paper, the critical strength of the UV flux above which the formation of molecular hydrogen remains suppressed was determined for a sample of five distinct haloes at z > 10 by employing a higher order chemical solver and a Jeans resolution of 32 cells.
Journal ArticleDOI
The impact of chemistry on the structure of high-z galaxies
Andrea Pallottini,Andrea Ferrara,Stefano Bovino,Livia Vallini,Simona Gallerani,Roberto Maiolino,Stefania Salvadori,Stefania Salvadori,Stefania Salvadori +8 more
TL;DR: In this article, the impact of H-2 chemistry on the evolution, morphology and observed properties of high-z galaxies has been studied using two zoom-in high-resolution (30 pc) simulati...