Properties after a fly-by
For extreme cases, there is no data available.
As part of the Fine Parameter Study, we have simulated the effect of a
stellar fly-by on a protoplanetary disk. The fly-by is modeled as a
perturber star passing by the host star and disk. A range of different
model parameters can be selected below. From the respective simulation
data, scatter plots and histograms are generated. The data of the Fine
Parameter Study can be downloaded
here.
To evaluate our results, we have compared them to the observed
properties of the known Trans-Neptunian Objects (TNOs). The data of
the TNOs can be downloaded from the Minor Planet Center:
distant_extended.json.gz
(Accessed on 2024/05/04 12:37)
This research has made use of data and/or services provided by the
International Astronomical Union's Minor Planet Center.
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