PS
Paolo Suin
astro-ph.GAastro-ph.IMastro-ph.SR
On Valency
published · living versionsW_m3zw62n9·v1 · currentpublished
What sets the star-formation rate in the Milky Way? I. A multi-scale view of the star-formation rate
with Patrick Hennebelle, Georges Abboudeh, Eugenio Schisano, Noé Brucy +13
1 version
Preprints & journals
8 papers in the corpus · 2022–2026The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO2606.26278v2 · A. Traficante, C. Mininni, F. Cavallaro et al.2026 · 0 citationsarXiv
MXDFz4.4: A LyC emitter 250Myr after the epoch of reionization and a first test of Ly-alpha morphology as a tracer of LyC escape at high redshift2603.04517v2 · Ilias Goovaerts, Marc Rafelski, Alexander Beckett et al.2026 · 0 citationsarXiv
Characterizing the interplay between Galactic star formation and ionization feedback with PRIMA2509.10654v1 · Annie Zavagno, Delphine Russeil, Paolo Suin et al.2025 · 0 citationsarXiv
The Rosetta Stone project. III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps2507.11032v1 · Alice Nucara, Alessio Traficante, Ugo Lebreuilly et al.2025 · 0 citationsarXiv
The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps2507.08436v2 · Ugo Lebreuilly, Alessio Traficante, Alice Nucara et al.2025 · 0 citationsarXiv
The role of magnetic field and stellar feedback in the evolution of filamentary structures in collapsing star-forming clouds2505.02903v1 · Paolo Suin, Doris Arzoumanian, Annie Zavagno et al.2025 · 10 citationsarXiv
Stellar Feedback in the Star Formation-Gas Density Relation: Comparison between Simulations and Observations2311.18522v1 · Paolo Suin, Annie Zavagno, Tine Colman et al.2023 · 10 citationsarXiv
Environmental Effects on the Dynamical Evolution of Star Clusters in Turbulent Molecular Clouds2207.01634v1 · Paolo Suin, Steven N. Shore, V'aclav Pavl'ik2022 · 5 citationsarXiv
Career total: 12 works. 8 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.