activity
20182023
most citedA new proxy to estimate the cosmic-ray ionisation rate in dense cores

34 citations · 102 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 28 cited

The GRETOBAPE gas-phase reaction network: the importance of being exothermic

Lorenzo Tinacci, Simón Ferrada-Chamorro, Cecilia Ceccarelli +5

The gas-phase reaction networks are the backbone of astrochemical models. However, due to their complexity and non-linear impact on the astrochemical modeling, they can be the firs…

astro-ph.SR2021★ 14 cited

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…

astro-ph.GA2020★ 34 cited

A new proxy to estimate the cosmic-ray ionisation rate in dense cores

Stefano Bovino, Simon Ferrada-Chamorro, Alessandro Lupi +2

Cosmic rays are a global source of ionisation, and the ionisation fraction represents a fundamental parameter in the interstellar medium. Ions couple to magnetic fields, affect the…

astro-ph.GA2019★ 26 cited

The 3D structure of CO depletion in high-mass prestellar regions

S. Bovino, S. Ferrada-Chamorro, A. Lupi +3

Disentangling the different stages of the star-formation process, in particular in the high-mass regime, is a challenge in astrophysics. Chemical clocks could help alleviating this…

astro-ph.GA2018

Synthetic observations of HD towards high-mass starless cores

Joaquin. Zamponi F., Dominik R. G. Schleicher, Stefano Bovino +3

Young massive stars are usually found embedded in dense and massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteratio…