activity
19992023
most citedOur astrochemical heritage

493 citations · 9.7k across the 174 of their papers we have counts for

collaborators

175 papers

astro-ph.GA2023

Quantum mechanical modeling of the grain-surface formation of acetaldehyde on HO:CO dirty ice surfaces

Jessica Perrero, Piero Ugliengo, Cecilia Ceccarelli +1

Acetaldehyde (CHCHO) is one of the most detected interstellar Complex Organic Molecule (iCOM) in the interstellar medium (ISM). These species have a potential biological releva…

astro-ph.GA2023★ 16 cited

SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys

Chentao Yang, Alain Omont, Sergio Martín +21

Understanding the nature of high- dusty galaxies requires a comprehensive view of their ISM and molecular complexity. However, the molecular ISM at high- is commonly studied…

astro-ph.GA2023★ 15 cited

Streamers feeding the SVS13-A protobinary system: astrochemistry reveals accretion shocks?

Eleonora Bianchi, Ana López-Sepulcre, Cecilia Ceccarelli +6

We report ALMA high-angular resolution (~ 50 au) observations of the binary system SVS13-A. More specifically, we analyse deuterated water (HDO) and sulfur dioxide (SO2) emission.…

astro-ph.GA2023★ 36 cited

Formation of complex organic molecules on interstellar CO ices? Insights from computational chemistry simulations

Stefano Ferrero, Cecilia Ceccarelli, Piero Ugliengo +2

Carbon (P) atom is a reactive species that, according to laboratory experiments and theoretical calculations, condensates with interstellar ice components. This fact is of utte…

astro-ph.SR2023★ 25 cited

FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA

S. Mercimek, L. Podio, C. Codella +25

More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…

astro-ph.SR2023★ 14 cited

FAUST VII. Detection of A Hot Corino in the Prototypical Warm Carbon-Chain Chemistry Source IRAS 15398-3359

Yuki Okoda, Yoko Oya, Logan Francis +16

We have observed the low-mass protostellar source, IRAS 153983359, at a resolution of 0.2-0.3, as part of the Atacama Large Millimeter/Submillimeter Array Large Program…