activity
20142024
most citedHow realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

102 citations · 344 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024

Testing analytical methods to derive the cosmic-ray ionisation rate in cold regions via synthetic observations

E. Redaelli, S. Bovino, A. Lupi +4

Cosmic rays (CRs) heavily impact the chemistry and physics of cold and dense star-forming regions. However, characterising their ionisation rate is still challenging from an observ…

astro-ph.GA202333 cited

First ALMA maps of cosmic ray ionisation rate in high-mass star-forming regions

Giovanni Sabatini, Stefano Bovino, Elena Redaelli

Low-energy cosmic rays ( TeV) are a pivotal source of ionisation of the interstellar medium, where they play a central role in determining the gas chemical composition and dras…

astro-ph.IM202245 cited

Binding Energy Evaluation Platform: A database of quantum chemical binding energy distributions for the astrochemical community

Giulia M. Bovolenta, Stefan Vogt-Geisse, Stefano Bovino +1

The quality of astrochemical models is highly dependent on reliable binding energy (BE) values that consider the morphological and energetic variety of binding sites on the surface…

astro-ph.GA202229 cited

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VI. The core-scale CO-depletion

Giovanni Sabatini, Stefano Bovino, Patricio Sanhueza +11

Studying the physical and chemical properties of cold and dense molecular clouds is crucial for the understanding of how stars form. Under the typical conditions of infrared dark c…

astro-ph.GA2014102 cited

How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

M. A. Latif, S. Bovino, T. Grassi +2

Observations of high redshift quasars at indicate that they harbor supermassive black holes (SMBHs) of a billion solar masses. The direct collapse scenario has emerged as the…

astro-ph.GA201420 cited

Effects of turbulence and rotation on protostar formation as a precursor to seed black holes

C. Van Borm, S. Bovino, M. A. Latif +3

Context. The seeds of the first supermassive black holes may have resulted from the direct collapse of hot primordial gas in K haloes, forming a supermassive or quas…