activity
20132025
most citedFAUST XVII: Super deuteration in the planet forming system IRS 63 where the streamer strikes the disk

20 citations · 60 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025

FAUST XXVII: The circumbinary disk and the outflow of the L 1551 IRS 5 binary system

Aurora Durán, Laurent Loinard, Pedro R. Rivera-Ortiz +21

Using continuum and line data obtained from the large ALMA program FAUST, we studied the structure of the protostellar binary system L1551 IRS5 at sc…

astro-ph.SR2025

Evidence for Jet/Outflow Shocks Heating the Environment Around the Class I Protostellar Source Elias 29: FAUST XXI

Yoko Oya, Eri Saiga, Anna Miotello +1

We have observed the late Class I protostellar source Elias~29 at a spatial-resolution of 70~au with the Atacama~Large~Millimeter/submillimeter~Array (ALMA) as part of the FAUST La…

astro-ph.GA2024

FAUST XIX. DCO in the outflow cavities of NGC\,1333 IRAS\,4A: recovering the physical structure of its original prestellar core

Layal Chahine, Cecilia Ceccarelli, Marta De Simone +25

Molecular deuteration is a powerful diagnostic tool for probing the physical conditions and chemical processes in astrophysical environments. In this work, we focus on formaldehyde…

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.,…

astro-ph.SR2024★ 8 cited

FAUST XV. A disk wind mapped by CHOH and SiO in the inner 300 au of the NGC 1333 IRAS 4A2 protostar

M. De Simone, L. Podio, L. Chahine +23

Context. Understanding the connection between outflows, winds, accretion and disks in the inner protostellar regions is crucial for comprehending star and planet formation process.…

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…

astro-ph.SR2024★ 13 cited

Anatomy of the Class I protostar L1489 IRS with NOEMA -- I. Disk, streamers, outflow(s) and bubbles at 3mm

M. Tanious, R. Le Gal, R. Neri +7

Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions…

astro-ph.SR2024

FAUST XI: Enhancement of the complex organic material in the shocked matter surrounding the [BHB2007] 11 protobinary system

C. Vastel, T. Sakai, C. Ceccarelli +20

iCOMs are species commonly found in the interstellar medium. They are believed to be crucial seed species for the build-up of chemical complexity in star forming regions as well as…

astro-ph.EP2013★ 19 cited

Evolution from protoplanetary to debris discs: The transition disc around HD 166191

G. M. Kennedy, S. J. Murphy, C. M. Lisse +12

HD 166191 has been identified by several studies as hosting a rare and extremely bright warm debris disc with an additional outer cool disc component. However, an alternative inter…