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Resolving galactic disks in their cosmic environment

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  3. ECOGAL Cloud comparison

Acknowledgement

Galactica database acknowledgement

If you use it in your own work, you may acknowledge the origin of the data obtained on the Galactica database like so:

This work reused datasets available on the Galactica simulations database
(http://www.galactica-simulations.eu)
                            
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NoĆ© BRUCY  

ECOGAL Cloud comparison

Summary

Cloud catalogs from ECOGAL ISM simulations used in Colman, Brucy, Girichidis et al. (subm.).

The extracted clouds come from multi-physics ISM simulations using a set of four different types of (M)HD simulations (SILCC, Girichidis 2021; LS, Colman et al. 2022; M51, Tress et al. 2021; Ramses-F20, Brucy 2022). The set covers a large range in spatial scales from 0.25 pc for the smallest cells in patches of the ISM up to a full galactic disks with a diameter of 30 kpc. Furthermore, the simulations were performed using different codes (Flash, Ramses and Arepo) with distinctive numerical techniques and physics ingredients of varying complexity.
For all data sets, we use a standardized 3D density-based extraction method build around the Hop algorithm.

The catalog will be uploaded in this page. An early version of the cloud catalog is available here.
The tools that were used to produced and analysed it are available here.

 

 

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This material is Open Data