activity
20182025
most citedAn image of the dust sublimation region in the nucleus of NGC 1068

115 citations · 257 across the 9 of their papers we have counts for

collaborators

13 papers

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

Unveiling accretion in the massive YSO G033.3891. Spatial and kinematic constraints from the CO bandhead emission

E. Koumpia, D. Sun, M. Koutoulaki +4

The inner parts of the hot discs surrounding massive young stellar objects (MYSOs) are still barely explored due to observational limitations in terms of angular resolution, scarci…

astro-ph.SR2023

The RMS survey: a census of massive YSO multiplicity in the -band

Robert G. Shenton, Rebecca J. Houghton, René D. Oudmaijer +4

Close to 100 per cent of massive stars are thought to be in binary systems. The multiplicity of massive stars seems to be intrinsically linked to their formation and evolution, and…

astro-ph.SR20221 cited

First spatially resolved Na I and He I transitions towards an MYSO. Finding new tracers for the gaseous star/disc interface

Evgenia Koumpia, M. Koutoulaki, W. -J. de Wit +4

With steady observational advances, the formation of massive stars is being understood in more detail. Numerical models are converging on a scenario where accretion discs play a ke…

astro-ph.SR202142 cited

A measure of the size of the magnetospheric accretion region in TW Hydrae

R. Garcia Lopez, A. Natta, A. Caratti o Garatti +69

Stars form by accreting material from their surrounding disks. There is a consensus that matter flowing through the disk is channelled onto the stellar surface by the stellar magne…

astro-ph.SR2021

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…