301 citations · 6.3k across the 162 of their papers we have counts for
8 papers · 1 filter
Non-ideal magnetohydrodynamics of self-gravitating filaments
Nicol Gutiérrez-Vera, Tommaso Grassi, Stefano Bovino +3
Filaments have been studied in detail through observations and simulations. A range of numerical works have separately investigated how chemistry and diffusion effects, as well as…
Formation of metal-free binaries: Impact of H line cooling and CIE cooling
Rafeel Riaz, Dominik R. G. Schleicher, Stefano Bovino +2
During primordial star formation, the main cooling channel is provided by H and super-molecules, such as H or H, at sufficiently high densities. When the latter f…
Role of magnetic fields in the formation of direct collapse black holes
Muhammad A. Latif, Dominik R. G. Schleicher, Sadegh Khochfar
Direct collapse black holes (DCBHs) are the leading candidates for the origin of the first supermassive black holes. However, the role of magnetic fields during their formation is…
Simulations of fully convective M dwarfs: dynamo action with varying magnetic Prandtl numbers
Carolina A. Ortiz-Rodríguez, Dominik R. G. Schleicher, Petri J. Käpylä +1
M dwarfs are low-mass main-sequence stars, the most numerous type of stars in the solar neighbourhood, which are known to have significant magnetic activity. The aim of this work i…
Synthetic observations using POLARIS: an application to simulations of massive prestellar cores
Joaquin Zamponi, Andrea Giannetti, Stefano Bovino +5
Young massive stars are usually found embedded in dense and massive molecular clumps which are known for being highly obscured and distant. During their formation process, the degr…
The Fermi paradox: Impact of astrophysical processes and dynamical evolution
Dominik R. G. Schleicher, Stefano Bovino
The Fermi paradox has given rise to various attempts to explain why no evidence of extraterrestrial civilisations was found so far on Earth and in our Solar System. Here, we presen…