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

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Showing astro-ph.GAShow all

5 papers · 1 filter

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.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.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.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 (…