activity
20222026
most citedValidation of 13 Hot and Potentially Terrestrial TESS Planets

34 citations · 100 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2026

Pristine composition or size evolution: Can current dust models reproduce emissivities observed in nearby protostars?

M. -A. Carpine, A. Maury, N. Ysard +1

Interstellar dust is a crucial asset in many astronomical observations. Characterising grains present in the dense gas and in star-forming environments is also key to constrain the…

astro-ph.GA2026

Jets and Outflows in Young Stellar Objects with the SKAO

Giovanni Sabatini, Gemma Busquet, Carlos Carrasco-González +48

Jets and outflows are ubiquitous phenomena associated with the formation of young stellar objects (YSOs). They play a crucial role in removing angular momentum from the accreting s…

astro-ph.SR2026

FAUST XXXI. Grain properties and variability of three sources in GSS 30

Q. Yang, H. Baobab Liu, S. Feng +55

To advance our understanding of dust properties in class 0/I young stellar objects, it is crucial to resolve their structures at multiple wavelengths and investigate how grain grow…

astro-ph.GA2026★ 1 cited

The environmental imprint on molecular layering in the dusty streamer of M512

M. De Simone, L. Cacciapuoti, D. Capela +7

Protostellar streamers are elongated structures that channel material from larger scale onto disks, influencing their physical and chemical evolution. The M512 protostar in Orion/L…

astro-ph.SR2025★ 4 cited

FAUST. XXVIII. High-Resolution ALMA Observations of Class 0/I Disks: Structure, Optical Depths, and Temperatures

M. J. Maureira, J. E. Pineda, H. B. Liu +22

We present high-resolution (~7.5 au) ALMA observations at 1.3 and 3 mm of 16 disks around Class 0/I protostars across multiple star-forming regions and a variety of multiplicities,…

astro-ph.GA2025

First results from ALPPS: a sub-Alfvénic streamer in SVS13A

P. C. Cortes, J. E. Pineda, T. -H. Hsieh +22

We present the first results from the ALMA Perseus Polarization Survey (ALPPS), focusing on the magnetic field in the SVS13A circumbinary disk. The dataset includes full-Stokes dus…

astro-ph.SR2025★ 9 cited

FAUST XXVI. The dust opacity spectral indices of protostellar envelopes bridge the gap between interstellar medium and disks

Luca Cacciapuoti, L. Testi, A. J. Maury +36

The sub-millimetre dust opacity spectral index is a critical observable to constrain dust properties, such as the maximum grain size of an observed dust population. It has been wid…

astro-ph.GA2025

FAUST XXIV. Large dust grains in the protostellar outflow cavity walls of the Class I binary L1551 IRS5

G. Sabatini, E. Bianchi, C. J. Chandler +19

Planet formation around young stars requires the growth of interstellar dust grains from mm-sized particles to km-sized planetesimals. Numerical simulations have shown that large (…

astro-ph.EP2025★ 14 cited

FAUST XX. The chemical structure and temperature profile of the IRAS 4A2 hot corino at 20-50 au

J. Frediani, M. De Simone, L. Testi +20

Young low-mass protostars often possess hot corinos, compact, hot and dense regions bright in interstellar Complex Organic Molecules (iCOMs). Besides of their prebiotic role, iCOMs…

astro-ph.SR2024

Planet Formation and Disk Chemistry: Dust and Gas Evolution during Planet Formation

G. Perotti, L. Cacciapuoti, N. -D. Tung +3

Over the past decade, progress in observational capabilities, combined with theoretical advancements, have transformed our comprehension of the physics and chemistry during planet…

astro-ph.EP2024★ 16 cited

Accuracy of ALMA estimates of young disk radii and masses. Predicted observations from numerical simulations

Ngo-Duy Tung, Leonardo Testi, Ugo Lebreuilly +7

Protoplanetary disks, which are the natural consequence of the gravitational collapse of the dense molecular cloud cores, host the formation of the known planetary systems in our u…

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.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…

astro-ph.EP2022★ 34 cited

Validation of 13 Hot and Potentially Terrestrial TESS Planets

Steven Giacalone, Courtney D. Dressing, Christina Hedges +108

The James Webb Space Telescope (JWST) will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify 18 potentially…