131 citations · 453 across the 16 of their papers we have counts for
32 papers
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…
The ALMA Survey of 70 Dark High-mass Clumps in Early Stages (ASHES). VII: Chemistry of Embedded Dense Cores
Shanghuo Li, Patricio Sanhueza, Xing Lu +15
We present a study of chemistry toward 294 dense cores in 12 molecular clumps using the data obtained from the ALMA Survey of 70 dark High-mass clumps in Early Stages (ASH…
Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
Stefano Bovino, Alessandro Lupi, Andrea Giannetti +4
Sun-like stars form from the contraction of cold and dense interstellar clouds. How the collapse proceeds and what are the main physical processes driving it, however, is still und…
Presence of water on exomoons orbiting free-floating planets: a case study
Patricio Javier Ávila, Tommaso Grassi, Stefano Bovino +4
A free-floating planet is a planetary-mass object that orbits around a non-stellar massive object (e.g. a brown dwarf) or around the Galactic Center. The presence of exomoons orbit…
Establishing the evolutionary timescales of the massive star formation process through chemistry
G. Sabatini, S. Bovino, A. Giannetti +6
(Abridged) Understanding the details of the formation process of massive (i.e. M<8-10M) stars is a long-standing problem in astrophysics. [...] We present a method to deriv…
Chemical post-processing of magneto-hydrodynamical simulations of star-forming regions: robustness and pitfalls
Simón Ferrada-Chamorro, Alessandro Lupi, Stefano Bovino
A common approach to model complex chemistry in numerical simulations is via post-processing of existing magneto-hydrodynamic simulations, relying on computing the evolution of che…