CLUES 2019 meeting in Lyon

The 2019 annual CLUES meeting and workshop will be held in Lyon, France, from 2-6 September 2019.
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CLUES Workshop 2018 in Puerto de la Cruz

The 2018 annual CLUES meeting and workshop will be held in Puerto de la Cruz, Tenerife, from 11-15 June 2018.
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CLUES Workshop 2017 in La Cristalera

Our next CLUES workshop takes  place in La Cristalera, from
June 19th  to June  23th,  2017.
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CLUES Workshop 2016 in Haifa, Israel

The CLUES Workshop 2016 was entitled “Cosmic Clues from the Near Field Universe” and took place in Israel.

See the workshop webpage for more details.

Date: 5-9, June 2016

Venue: Bay Club Haifa Hotel, Haifa, Israel
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Box 64 – 186592 – gas in MW at z=0

Gas distribution of the Milky Way (Box 64 – 186592, 4096^3 particles resimulation), at redshift z=0.0, colored by density.

Credits: K. Riebe; PMViewer

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Box 64 – 186592 – gas in M31, MW and M33 at z=0

Box 64 – 186592 – gas in M31, MW and M33 at z=0

Gas distribution of the three main galaxies at z=0.0 (Box 64 – 186592), colored by temperature.

Credits: A. Khalatyan; PMViewer

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Box 64 – 186592 – gas in M31, MW and M33 at z=0.84

Box 64 – 186592 – gas in M31, MW and M33 at z=0.84

Gas distribution of the three main galaxies M31, Milky Way and M33 (Box 64 – 186592), at z = 0.84, colored by density.

Credits: A. Khalatyan; PMViewer

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Box 64 – 186592 – gas in M33 at z=0.78

Box 64 – 186592 – gas in M33 at z=0.78

Gas distribution of M33 (Box 64 – 186592), at redshift z = 0.78, colored by density.

Credits: A. Khalatyan; PMViewer

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Box 64 – 186592 – gas in M31 at z=0.78

Box 64 – 186592 – gas in M31 at z=0.78

View on the gas distribution of M31 (Box 64 – 186592), at redshift z = 0.78, colored by density.

Credits: A. Khalatyan; PMViewer

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Box 64 – 186592 – gas in LG and M33 (hi-res)

Box 64 – 186592 – gas in LG and M33 (hi-res)

A view on the Local Group (along the z-axis of the simulation box, Box 64 – 186592, 4096^3 particles effective resolution) with a flight to M33 from a distance of ~ 3.3 Mpc/h to 300 kpc/h (redshift z=0).
Colors reflect the gas density (brighter = higher density).
The first seconds of the movie show the dark matter distribution of the Local Group for comparison.

Credits: K. Riebe; PMViewer

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