activity
19992022
most citedFirst detection of triply-deuterated methanol

261 citations · 2.6k across the 62 of their papers we have counts for

collaborators
Showing 2018Show all

15 papers · 1 filter

astro-ph.EP2018

A theoretical investigation of the reaction between the amidogen, NH, and the ethyl, C2H5, radicals: a possible gas-phase formation route of interstellar and planetary ethanimine

Nadia Balucani, Dimitrios Skouteris, Cecilia Ceccarelli +3

The reaction between the amidogen, NH, radical and the ethyl, C2H5, radical has been investigated by performing electronic structure calculations of the underlying doublet potentia…

astro-ph.GA2018

Interstellar dimethyl ether gas-phase formation: a quantum chemistry and kinetics study

Dimitrios Skouteris, Nadia Balucani, Cecilia Ceccarelli +4

Dimethyl ether is one of the most abundant interstellar complex organic molecules. Yet its formation route remains elusive. In this work, we have performed electronic structure and…

astro-ph.EP2018

Can Formamide Be Formed on Interstellar Ice? An Atomistic Perspective

Albert Rimola, Dimitrios Skouteris, Nadia Balucani +4

Interstellar formamide (NH2CHO) has recently attracted significant attention due to its potential role as a molecular building block in the formation of precursor biomolecules rele…

astro-ph.GA2018

Rotation in the NGC 1333 IRAS 4C Outflow

Yichen Zhang, Aya E. Higuchi, Nami Sakai +8

We report molecular line observations of the NGC 1333 IRAS 4C outflow in the Perseus Molecular Cloud with the Atacama Large Millimeter/Submillimeter Array. The CCH and CS emission…

astro-ph.SR2018

First Hot Corino detected around an Isolated Intermediate-Mass Protostar: Cep\,E-mm

J. Ospina Zamudio, B. Lefloch, C. Ceccarelli +4

Intermediate-mass (IM) protostars provide a bridge between the low- and high-mass protostars. Despite their relevance, little is known about their chemical diversity. We want to in…

astro-ph.GA2018

IR Spectral Fingerprint of Carbon Monoxide in Interstellar Water Ice Models

Lorenzo Zamirri, Silvia Casassa, Albert Rimola +3

Carbon monoxide (CO) is the second most abundant molecule in the gas-phase of the interstellar medium. In dense molecular clouds, it is also present in the solid-phase as a constit…