21 citations · 65 across the 6 of their papers we have counts for
6 papers
HYPERION. The cold ISM of rapidly growing quasars: diverse gas reservoirs, dust enrichment, and feedback signatures
Claudia Maria Pierro, Roberta Tripodi, Laura Pentericci +11
Luminous QSOs at host some of the most rapidly assembled SMBHs in the early Universe. Characterizing their cold ISM is essential to determine their evolution. We investigate…
ALMA 360 pc high-frequency observations reveal warm dust in the center of a quasar
Romain A. Meyer, Fabian Walter, Fabio Di Mascia +3
The temperature of the cold dust in z>6 galaxies is a potential tracer of Active Galactic Nucleus (AGN) and stellar feedback, and is the dominant source of uncertainty in inferring…
ALMA observations of super-early galaxies: attenuation-free model predictions
A. Ferrara, S. Carniani, F. di Mascia +3
The abundance and blue color of super-early (redshift ), luminous galaxies discovered by JWST can be explained if radiation-driven outflows have ejected their dust on kpc-sca…
Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
Fabio Di Mascia, Andrea Pallottini, Laura Sommovigo +1
Context. Molecular Clouds (MCs) are the place where stars are formed and their feedback starts to take place, regulating the evolution of galaxies. Therefore, MCs represent the cri…
Is the star formation rate in quasars overestimated?
Fabio Di Mascia, Stefano Carniani, Simona Gallerani +4
The large total infrared (TIR) luminosities () observed in quasars are generally converted into high star formation rates ($SFR \gtr…
Enhanced star formation in quasar companions
Tommaso Zana, Simona Gallerani, Stefano Carniani +5
Quasars powered by supermassive black holes (MBH, ) at are predicted to reside in cosmic over-dense regions. However, observations so far could not confi…