372 citations · 6.2k across the 119 of their papers we have counts for
17 papers · 1 filter
Observing planetesimal formation under streaming instability in the rings of HD 163296
Francesco Zagaria, Cathie J. Clarke, Richard A. Booth +2
We introduce a new technique to determine the gas turbulence and surface density in bright disc rings, under the assumption that dust growth is limited by turbulent fragmentation a…
The external photoevaporation of structured protoplanetary disks
Matías Gárate, Paola Pinilla, Thomas J. Haworth +1
The dust in planet-forming disks evolve rapidly through growth and radial drift, and external photoevaporation also contributes to this evolution in massive star-forming regions. W…
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): HD 34700 A unveils an inner ring
G. Columba, E. Rigliaco, R. Gratton +18
Context. The study of protoplanetary disks is fundamental to understand their evolution and interaction with the surrounding environment, and to constrain planet formation mechanis…
Protoplanetary disks in -band total intensity and polarized light
Bin B. Ren, Myriam Benisty, Christian Ginski +11
Diverse protoplanetary disk morphology can result from planet-disk interaction, suggesting planetary presence. To date, most scattered light imaging campaigns have probed polarized…
Protoplanetary Disk Chemistry
Karin I. Öberg, Stefano Facchini, Dana E. Anderson
Planets form in disks of gas and dust around young stars. The disk molecular reservoirs and their chemical evolution affect all aspects of planet formation, from the coagulation of…
MagAO-X and HST high-contrast imaging of the AS209 disk at H
Gabriele Cugno, Yifan Zhou, Thanawuth Thanathibodee +22
The detection of emission lines associated with accretion processes is a direct method for studying how and where gas giant planets form, how young planets interact with their nata…