activity
20172026
most citedSeeds Of Life In Space (SOLIS): The organic composition diversity at 300--1000 au scale in Solar-type star forming regions

155 citations · 873 across the 29 of their papers we have counts for

collaborators
Showing 2024Show all

7 papers · 1 filter

astro-ph.GA2024★ 1 cited

Role of NH3 Binding Energy in the Early Evolution of Protostellar Cores

S. Kakkenpara Suresh, O. Sipila, P. Caselli +1

NH(ammonia) plays a critical role in the chemistry of star and planet formation, yet uncertainties in its binding energy (BE) values complicate accurate estimates of its abun…

astro-ph.EP2024★ 20 cited

FAUST XVII: Super deuteration in the planet forming system IRS 63 where the streamer strikes the disk

L. Podio, C. Ceccarelli, C. Codella +55

Recent observations suggest that planets formation starts early, in protostellar disks of yrs, which are characterized by strong interactions with the environment, e.g.,…

physics.chem-ph2024★ 7 cited

Binding energies of ethanol and ethylamine on interstellar water ices: synergy between theory and experiments

Jessica Perrero, Julie Vitorino, Emanuele Congiu +3

Experimental and computational chemistry are two disciplines to conduct research in Astrochemistry, providing essential reference data for both astronomical observations and modeli…

astro-ph.GA2024

Multiple chemical tracers finally unveil the intricate NGC\,1333 IRAS\,4A outflow system. FAUST XVI

Layal Chahine, Cecilia Ceccarelli, Marta De Simone +54

The exploration of outflows in protobinary systems presents a challenging yet crucial endeavour, offering valuable insights into the dynamic interplay between protostars and their…

astro-ph.GA2024

Comprehensive laboratory constraints on thermal desorption of interstellar ice analogues

F. Kruczkiewicz, F. Dulieu, A. V. Ivlev +4

To explain grain growth and destruction in warm media, ice mantle formation and sublimation in cold media, and gas line emission spectroscopy, astrochemical models must mimic the g…

astro-ph.GA2024

FAUST XIII. Dusty cavity and molecular shock driven by IRS7B in the Corona Australis cluster

G. Sabatini, L. Podio, C. Codella +54

The origin of the chemical diversity observed around low-mass protostars probably resides in the earliest history of these systems. We aim to investigate the impact of protostellar…