293 citations · 5.8k across the 121 of their papers we have counts for
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Sub-mm/mm optical properties of real protoplanetary matter derived from Rosetta/MIRO observations of comet 67P
Johanna Bürger, Thilo Glißmann, Anthony Lethuillier +6
Optical properties are required for the correct understanding and modelling of protoplanetary and debris discs. By assuming that comets are the most pristine bodies in the solar sy…
On the underestimation of dust mass in protoplanetary disks: Effects of disk structure and dust properties
Yao Liu, Hendrik Linz, Min Fang +6
The total amount of dust grains in protoplanetary disks is one of the key properties that characterize the potential for planet formation. With (sub-)millimeter flux measurements,…
Hot exozodis: cometary supply without trapping is unlikely to be the mechanism
Tim D. Pearce, Florian Kirchschlager, Gaël Rouillé +6
Excess near-infrared emission is detected around one fifth of main-sequence stars, but its nature is a mystery. These excesses are interpreted as thermal emission from populations…
Locating dust and molecules in the inner circumstellar environment of R~Sculptoris with MATISSE
Julien Drevon, Florentin Millour, Pierre Cruzalèbes +49
AGB stars are one of the main sources of dust production in the Galaxy. However, it is not clear what this process looks like and where the dust is condensing in the circumstellar…
Millimeter Gap Contrast as a Probe for Turbulence Level in Protoplanetary Disks
Yao Liu, Gesa H. -M. Bertrang, Mario Flock +7
Turbulent motions are believed to regulate angular momentum transport and influence dust evolution in protoplanetary disks. Measuring the strength of turbulence is challenging thro…
Radiative transfer simulations for in-situ particle size diagnostic in reactive, particle growing plasmas
Julia Kobus, Andreas Petersen, Franko Greiner +1
When considering particles produced in reactive plasmas, their basic properties, such as refractive index and grain size often need to be known. They can be constrained both ex-sit…