activity
20092024
most citedZooming on the internal structure of galaxies

135 citations · 670 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2024★ 8 cited

Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe

Alessandro Trinca, Rosa Valiante, Raffaella Schneider +7

Early JWST observations are providing growing evidence for a ubiquitous population of accreting supermassive black holes (BHs) at high redshift, many of which appear overmassive co…

astro-ph.GA2023★ 3 cited

Are we surprised to find SMBHs with JWST at z > 9?

Raffaella Schneider, Rosa Valiante, Alessandro Trinca +3

JWST is unveiling for the first time accreting black holes (BHs) with masses of 10^6 - 10^7 Msun at z > 4, with the most distant residing in GNz11 at z = 10.6. Are we really surpri…

astro-ph.GA2022★ 43 cited

Seeking the growth of the first black hole seeds with JWST

Alessandro Trinca, Raffaella Schneider, Roberto Maiolino +3

In this paper we provide predictions for the BH population that would be observable with planned JWST surveys at . We base our study on the recently developed Cosmi…

astro-ph.GA2016★ 135 cited

Zooming on the internal structure of galaxies

A. Pallottini, A. Ferrara, S. Gallerani +3

We present zoom-in, AMR, high-resolution ( pc) simulations of high-redshift () galaxies with the aim of characterizing their internal properties and interste…

astro-ph.GA2016★ 85 cited

ALMA suggests outflows in z~5.5 galaxies

S. Gallerani, A. Pallottini, C. Feruglio +5

We present the first attempt to detect outflows from galaxies approaching the Epoch of Reionization (EoR) using a sample of 9 star-forming () $z…

astro-ph.SR2013★ 49 cited

Dust formation in the winds of AGBs: the contribution at low metallicities

Marcella Di Criscienzo, Flavia Dell'Agli, Paolo Ventura +6

We present new models for the evolution of stars with mass in the range 1Msun < M < 7.5Msun, followed from the pre-main-sequence through the asymptotic giant branch phase. The meta…