![](http://hestia.aip.de/wp-content/uploads/2020/05/DM_COM_img_37_11_0_127___0000.png)
![](http://hestia.aip.de/wp-content/uploads/2020/05/cropped-gas_Eon_17_11_halo1_127.png)
![](http://hestia.aip.de/wp-content/uploads/2020/05/cropped-17_11_0_y-2.jpg)
Full 1
the simulations
HESTIA
High-resolution Environmental Simulations of The Immediate Area
High-resolution Environmental Simulations of The Immediate Area
![Full 1](http://hestia.aip.de/wp-content/uploads/slider2/f1.jpg)
Full 2
Stars, gas and dark matter
Gas and the Local Group's circumgalactic medium
![Full 2](http://hestia.aip.de/wp-content/uploads/slider2/f2.jpg)
Full 3
The Local Group
Spiral Milky Way and Andromeda galaxies
![Full 3](http://hestia.aip.de/wp-content/uploads/slider2/f3.jpg)
![](https://hestia.aip.de/wp-content/uploads/2020/05/gas_Fon_17_11_halo0_127-1.png)
About The Team
The HESTIA suite of simulations is a collaboration of collaborations: from the CosmicFlows team which compiles galaxy distances, to the CLUES collaboration which generates constrained initial conditions, to the AURIGA model of galaxy formation that employs the AREPO hydrosolver.
![](https://hestia.aip.de/wp-content/uploads/2020/05/hestia-for-noam-2-_inverted.jpg)