611 citations · 8.6k across the 104 of their papers we have counts for
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Mass constraints for 15 protoplanetary disks from HD 1-0
M. Kama, L. Trapman, D. Fedele +6
Hydrogen deuteride (HD) rotational line emission can provide reliable protoplanetary disk gas mass measurements, but it is difficult to observe and detections have been limited to…
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…
A dust and gas cavity in the disc around CQ Tau revealed by ALMA
M. Giulia Ubeira Gabellini, Anna Miotello, Stefano Facchini +23
The combination of high resolution and sensitivity offered by ALMA is revolutionizing our understanding of protoplanetary discs, as their bulk gas and dust distributions can be stu…
Gas vs dust sizes of protoplanetary disks: effects of dust evolution
L. Trapman, S. Facchini, M. R. Hogerheijde +2
The extent of the gas in protoplanetary disks is observed to be universally larger than the extent of the dust. This is often attributed to radial drift and grain growth of the mm…