activity
20172022
most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

201 citations · 339 across the 5 of their papers we have counts for

collaborators

11 papers

astro-ph.SR202237 cited

The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

C. C. Espaillat, G. J. Herczeg, T. Thanathibodee +59

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data fro…

astro-ph.SR202214 cited

The accretion process in the DQ Tau binary system

Eleonora Fiorellino, Sunkyung Park, Ágnes Kóspál +1

Mass accretion from the circumstellar disk onto the protostar is a fundamental process during star formation. Measuring the mass accretion rate is particularly challenging for star…

astro-ph.GA2021

The Hi-GAL compact source catalogue -- II. The 360° catalogue of clump physical properties

D. Elia, M. Merello, S. Molinari +29

We present the catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 m. This release not only completes the analogous catalogue pre…

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…

astro-ph.SR2021

KMOS study of the mass accretion rate from Class I to Class II in NGC 1333

Eleonora Fiorellino, Carlo Felice Manara, Brunella Nisini +6

The mass accretion rate is the fundamental parameter to understand the process of mass assembly that results in the formation of a low-mass star. This parameter has been largely st…

astro-ph.GA202039 cited

Mass segregation and sequential star formation in NGC 2264 revealed by Herschel

T. Nony, J. -F. Robitaille, F. Motte +16

The mass segregation of stellar clusters could be primordial rather than dynamical. Despite the abundance of studies of mass segregation for stellar clusters, those for stellar pro…