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A Photoionized Accretion Disk around a Young High-mass Star
(IOP, 2020)
We present high spatial resolution (52 au) observations of the high-mass young stellar object (HMYSO) G345.4938+01.4677 made using the Atacama Large Millimeter/submillimeter Array. This O-type HMYSO is located at 2.38 kpc ...
Compact Dust Concentration in the MWC 758 Protoplanetary Disk
(The American Astronomical Society, 2015-11-01)
The formation of planetesimals requires that primordial dust grains grow from micron- to kilometer-sized bodies.
Dust traps caused by gas pressure maxima have been proposed as regions where grains can concentrate and ...
Compact dust concentration in the mwc 758 protoplanetary disk
(IOP Publishing, 2015)
The formation of planetesimals requires that primordial dust grains grow from micron- to km-sized bodies.
Dust traps caused by gas pressure maxima have been proposed as regions where grains can concentrate and
grow fast ...
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 ...
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 ...
The kuperberg conjecture is true in two dimensions: any strictly compact C2 figure can be fixed firmly by three points unless it is the disk
(Centro de Investigación y Docencia Económicas, 2011)
The kuperberg conjecture is true in two dimensions: any strictly compact C2 figure can be fixed firmly by three points unless it is the disk
(Centro de Investigación y Docencia Económicas, 2011)
High-resolution observations of the outer disk around T Chamaeleontis: the view from ALMA
(EDP Sciences, 2015)
Context. Transitional disks are circumstellar disks with dust gaps thought to be related in some cases to planet formation. They can
shed light on the planet formation process by the analysis of their gas and dust properties. ...