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Shadows cast by a warp in the HD 142527 protoplanetary disk
(IOP Publisihing, 2015)
Detailed observations of gaps in protoplanetary disks have revealed structures that drive current research on circumstellar disks. One such feature is the two intensity nulls seen along the outer disk of the HD 142527 ...
Shadows Cast by a Warp in the HD 142527 Protoplanetary Disk
(The American Astronomical Society, 2015-01-10)
Detailed observations of gaps in protoplanetary disks have revealed structures that drive current research on
circumstellar disks. One such feature is the two intensity nulls seen along the outer disk of the HD 142527 ...
Multiwavelength optical properties of compact dust aggregates in protoplanetary disks
(EDP SCIENCES, 2016)
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with complex shapes and compositions. The coagulation process changes the absorption and scattering properties of particles in ...
The widest Hα survey of accreting protoplanets around nearby transition disks
(EDP Sciences, 2020)
Protoplanetary Disks Including Radiative Feedback from Accreting Planets
(The American Astronomical Society, 2015)
While recent observational progress is converging on the detection of compact regions of thermal emission due to
embedded protoplanets, further theoretical predictions are needed to understand the response of a ...
Dust trapping around Lagrangian points in protoplanetary disks
(European Southern Observatory, 2020)
Aims. Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points L4 and L5. In the Solar System, these bodies show a broad size distribution ranging from micrometer (μm) to centimeter ...
Giant Planets Can Act as Stabilizing Agents on Debris Disks
(2017-07-01)
We have explored the evolution of a cold debris disk under the gravitational influence of dwarf-planet-sized objects (DPs), both in the presence and absence of an interior giant planet. Through detailed long-term numerical ...
Redistribution of CO at the location of the CO ice line in evolving gas and dust disks
(EDP SCIENCES S A, 2017)
Context. Ice lines are suggested to play a significant role in grain growth and planetesimal formation in protoplanetary disks. Evaporation fronts directly influence the gas and ice abundances of volatile species in the ...