activity
20242026
collaborators

8 papers

astro-ph.SR2026

Hunting for methanol in the water rich, planet forming disk around HL Tau

Alessandro Soave, Margot Leemker, Stefano Facchini +3

Methanol, the simplest complex organic molecule found in space, is considered a key compound necessary for the formation of chemical species of prebiotic interest. Methanol detecti…

astro-ph.EP2026

Zooming into the water snowline: high resolution water observations of the HL Tau disk

M. Leemker, S. Facchini, P. Curone +4

Water is one of the central molecules for the formation and habitability of planets. In particular, the region where water freezes-out, the water snowline, could be a favorable loc…

astro-ph.EP2025

The chemical diversity of giant-planet nurseries as revealed by ALMA

Alice S. Booth, Jenny Calahan, Milou Temmink +9

With the giant exoplanet occurrence rate peaking around stars of 1.5-2 solar masses, there is strong motivation to characterize the disks that set their formation conditions. Obser…

astro-ph.EP2025

Pristine ices in a planet-forming disk revealed by heavy water

Margot Leemker, John J. Tobin, Stefano Facchini +4

Water is essential to our understanding of the planet-formation process and habitability on Earth. Although trace amounts of water are seen across all phases of star and planet for…

astro-ph.EP2025

Ice sublimation in the dynamic HD 100453 disk reveals a rich reservoir of inherited complex organics

Alice S. Booth, Lisa Wölfer, Milou Temmink +7

Protoplanetary disks around luminous young A-type stars are prime observational laboratories to determine the abundances of complex organic molecules (COMs) present during planet f…

astro-ph.EP2025

Radial variations in nitrogen, carbon, and hydrogen fractionation in the PDS 70 planet-hosting disk

L. Rampinelli, S. Facchini, M. Leemker +8

Element isotopic ratios are powerful tools to reconstruct the journey of planetary material, from the parental molecular cloud to protoplanetary disks, where planets form and accre…