Supercomputing and E-Science Visualisation

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Gas distribution in Local group, CLUES B64_WM3

The image/movie shows the distribution of gas in the CLUES simulation B64_WM3_186592, a resimulation with 40963 particles, rendered with PMViewer. Colors represent the density of gas, from dark blue for sparse to bright yellow for very dense regions. The resimulated area was chosen because of its similarity to the Local Group, with Andromeda (M31) in the center, M33 to the lower right and the Milky Way at the upper right corner.

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MW vs M31, Box64 LG, 2048^3

Box64 LG, 2048^3 effective particles, Resimulated region size: 2Mpc/h

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Fly by movie showing the distribution

Fly by movie showing the distribution of RAVE stars 200Myrs ago compared to the Milky Way disk.

Distances by Breddels et al 2009.

Movie by Gal Matijevic.

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Fly by movie

Fly by movie showing the distribution of RAVE stars compared to the Milky Way disk.

Distances by Breddels et al 2009. Movie by Gal Matijevic.

 

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Cosmological formation of a elliptical galaxy (20kpc box)

Reference: Steinmetz & Navarro, 2002, New Astronomy, 7, 155640×480 MPEG @ 10fps (12.1MB)

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