activity
20032026
most citedAn Imprint of Molecular Cloud Magnetization in the Morphology of the Dust Polarized Emission

262 citations · 1.1k across the 66 of their papers we have counts for

collaborators
Showing 2023Show all

7 papers · 1 filter

astro-ph.GA2023

Stellar Feedback in the Star Formation-Gas Density Relation: Comparison between Simulations and Observations

Paolo Suin, Annie Zavagno, Tine Colman +3

Context. The impact of stellar feedback on the Kennicutt-Schmidt law (KS law), which relates star formation rate (SFR) to surface gas density, is a topic of ongoing debate. The int…

astro-ph.EP2023

Protostellar chimney flues: are jets and outflows lifting submillimetre dust grains from discs into envelopes?

L. Cacciapuoti, L. Testi, L. Podio +7

Low dust opacity spectral indices () measured in the inner envelopes of class 0/I young stellar objects (age yr) have been interpreted as the presence of (sub…

astro-ph.EP2023

A dusty streamer infalling onto the disk of a class I protostar. ALMA dual-band constraints on grain properties and mass infall rate

L. Cacciapuoti, E. Macias, A. Gupta +15

Observations of interstellar material infalling onto star- and planet-forming systems have become increasingly common thanks to recent advancements in radio interferometry. These s…

astro-ph.IM2023

Environmental transition: overview of actions to reduce the environmental footprint of astronomy

Lucie Leboulleux, Faustine Cantalloube, Marie-Alice Foujols +15

To keep current global warming below 1.5°C compared with the pre-industrial era, measures must be taken as quickly as possible in all spheres of society. Astronomy must also make i…

astro-ph.SR2023★ 1 cited

Synthetic populations of protoplanetary disks. Impact of magnetic fields and radiative transfer

U. Lebreuilly, P. Hennebelle, T. Colman +10

Protostellar disks are the product of angular momentum conservation during the protostellar collapse. Understanding their formation is crucial because they are the birthplace of pl…

astro-ph.SR2023★ 22 cited

FAUST IX. Multi-band, multi-scale dust study of L1527 IRS. Evidence for dust properties variations within the envelope of a Class 0/I YSO

L. Cacciapuoti, E. Macias, A. J. Maury +25

Early dust grain growth in protostellar envelopes infalling on young discs has been suggested in recent studies, supporting the hypothesis that dust particles start to agglomerate…