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Jupiter formed as a pebble pile around the N ice line
Arthur D. Bosman, Alex J. Cridland, Yamila Miguel
The region around the HO ice line, due to its higher surface density, seems to be the ideal location to form planets. The core of Jupiter, as well as the cores of close in gas…
The dry and carbon poor inner disk of TW Hya: evidence for a massive icy dust trap
Arthur D. Bosman, Andrea Banzatti
Gas giants accrete their envelopes from the gas and dust of proto-planetary disks, so it is important to determine the composition of the inner few AU, where most giant planets are…
HCN/HNC intensity ratio: a new chemical thermometer for the molecular ISM
A. Hacar, A. D. Bosman, E. F. van Dishoeck
Context. The gas kinetic temperature (TK) determines the physical and chemical evolution of the Interestellar Medium (ISM). However, obtaining reliable TK estimates usually require…
Probing planet formation and disk substructures in the inner disk of Herbig Ae stars with CO rovibrational emission
Arthur D. Bosman, Andrea Banzatti, Simon Bruderer +3
[abridged]CO rovibrational lines are efficient probes of warm molecular gas and can give unique insights into the inner 10 AU of proto-planetary disks. Recent studies have found a…