3D Temperature Distribution in our Coma Cluster Simulation
3D Temperature Distribution

High Resolution Picture
(143
KB)

143 KB
Plan view Movie
(Indeo 5.10)
(~8.7 MB)
ca. 8.7 MB

Plan view Movie
(DivX 4)
(384
KB)

384 KB
Plan view Movie
(MPEG)
(7.17 M
B)
7.17 MB
Rotation Movie
(Indeo 5.10)
(~16 MB)
ca. 16 MB

Rotation Movie
(DivX 4)
(2
MB)

384 KB

Rotation Movie
(MPEG)
(9
MB)

9 MB
3D Temperature Distribution

High Resolution Picture
(102
KB)

102 KB
Plan view Movie
(Indeo 5.10)
(~8.95 MB)
ca. 8.9 MB

Plan view Movie
(DivX 4)
(422
KB)

422 KB

Plan view Movie
(MPEG)
(7.45 MB
)

7.45 MB
Rotation Movie
(Indeo 5.10)
(~15 MB)
ca. 15 MB

Rotation Movie
(DivX 4)
(1.66 M
B)

1.66 MB

Rotation Movie
(MPEG)
(8.7 M
B)

8.7 MB
3D Temperature Distribution

High Resolution Picture
(107
KB)

107 KB
Plan view Movie
(Indeo 5.10)
(10 MB)
10 MB

Plan view Movie
(DivX 4)
(608
KB)

608 KB

Plan view Movie
(MPEG)
(7.78 MB
)

7.78 MB
Rotation Movie
(Indeo 5.10)
(16.3 MB)
16.3 MB

Rotation Movie
(DivX 4)
(1.9 M
B)

1.9 MB

Rotation Movie
(MPEG)
(8.92 M
B)

8.92 MB
3D Temperature Distribution

High Resolution Picture
(170
KB)

170 KB
Plan view Movie
(Indeo 5.10)
(~11 MB)
10.8 MB

Plan view Movie
(DivX 4)
(772
KB)

772 KB

Plan view Movie
(MPEG)
(7.8 MB
)

7.8 MB
Rotation Movie
(Indeo 5.10)
(~16 MB)
16 MB

Rotation Movie
(DivX 4)
(2 MB
)

2 MB

Rotation Movie
(MPEG)
(8.92 MB
)

8.92 MB
Temperature distribution in the Coma cluster simulation. Outgoing shock fronts caused by subcluster mergers are shown. In the highest resolution the cold stripped gas from galaxies can be seen.
 
Institute for Astrophysics, University of Innsbruck