3 citations · 13 across the 13 of their papers we have counts for
8 papers · 1 filter
Dusty substructures induced by planets in ALMA disks: how dust growth and dynamics changes the picture
Alexandros Ziampras, Prakruti Sudarshan, Cornelis P. Dullemond +4
Protoplanetary disks exhibit a rich variety of substructure in millimeter continuum emission, often attributed to unseen planets. As these planets carve gaps in the gas, dust parti…
UV-processing of icy pebbles in the outer parts of VSI-turbulent disks
Lizxandra Flores-Rivera, Michiel Lambrechts, Sacha Gavino +4
Icy dust particles emerge in star-forming clouds and are subsequently incorporated in protoplanetary disks, where they coagulate into larger pebbles up to mm in size. In the disk m…
Variability of the inner dead zone edge in 2D radiation hydrodynamic simulations
Michael Cecil, Mario Flock
The inner regions of protoplanetary disks are prone to thermal instability (TI), which can significantly impact the thermal and dynamic evolution of planet-forming regions. Observa…
Dust mass in protoplanetary disks with porous dust opacities
Yao Liu, Hélène Roussel, Hendrik Linz +8
ALMA surveys have suggested that protoplanetary disks are not massive enough to form the known exoplanet population, under the assumption that the millimeter continuum emission is…
From traffic jams to roadblocks: The outer regions of TW Hya with ALMA Band 8
Sreejita Das, Nicolas T. Kurtovic, Mario Flock
We present Atacama Large Millimeter Array (ALMA) observations of TW Hya at 0.65 mm with 0.5 arcsecond angular resolution, together with high angular resolution archival observation…
Support for fragile porous dust in a gravitationally self-regulated disk around IM Lup
Takahiro Ueda, Ryo Tazaki, Satoshi Okuzumi +2
Protoplanetary disks, the birthplace of planets, are expected to be gravitationally unstable in their early phase of evolution. IM Lup, a well-known T-Tauri star, is surrounded by…