Name/Topic
|
Files |
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Clemens: Club of Rome |
CoR.key
|
Clemens: Deutsches Museum |
DM.key
|
Clemens: Staunen und Verstehen |
Staunen.key
|
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Alvaro: Infall of stellar stream: x-y distribution |
xy.gif
|
Alvaro: Infall of stellar stream: x - velocity distribution |
xv.gif
|
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Aaron: UDG formation: somewhat less mass loss |
udg1.gif
|
Aaron: UDG formation: somewhat more mass loss |
udg2.gif
|
Aaron: UDG formation: z-distribution |
uz.gif
|
|
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Doug: Nbody collapse of elongated structure |
collapse1.gif
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Doug: Nbody collapse of elongated structure: larger environment |
collapse2.gif
|
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Jens: Hernquist initial distribution with larger separation |
penergy_h_20.init
|
Jens: Hernquist final distribution with larger separation |
penergy_h_20.final
|
Jens: Plummer collapse; t=0 |
pcoll.init
|
Jens: Plummer collapse; t=40 |
pcoll.40
|
Jens: Plummer resim; t=0 |
plum.resim.0
|
Jens: Plummer resim: t=40 |
plum.resim.200
|
Jens: penergy_h.180 |
penergy_h.180
|
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Graeme: cluster merger |
cluster.gif
|
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rho = constant; extreme case |
dm6.gif
|
Joe: rho = 1/r**2 |
dm1.gif
|
Joe: rho = 1/r |
dm2.gif
|
Joe: rho = constant |
dm3.gif
|
Joe: rho = constant, eccentric orbit |
dm4.gif
|
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Galactic disk evolution: Dobbs et al. |
disk.mov
|
Clare: self-regulated star formation |
starformation.key
|
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Population evolution within a globular cluster |
cluster.gif
|
Population evolution: seeding and mortality |
cluster1.gif
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Population evolution: seeding and loss of resources |
cluster2.gif
|
Population evolution: seeding, exhaustion, stellar evolution, star formation |
cluster3.gif
|
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|
HCC087 on an almost circular orbit |
circular.gif
|
2-component model of HCC087 around cluster center |
baryon.gif
|
HCC087 around HCC005 |
hcc087.gif
|
HCC087 around HCC005 (zoom) |
zoom.gif
|
HCC087 around Cluster center |
animcc.gif
|
HCC087 around Cluster center (zoom) |
zoomcc.gif
|
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ppt Folien fuer Thomas |
thomas.ppt
|
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G2 movie |
g2.mp4
|
G2 talk (pdf) |
g2.pdf
|
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Internal dynamics of a stable 3:1 filament (xy-plane: x: long axis): |
3to1_xy.gif
|
3:1 stable filament (yz-plane, perpendicular to long axis): |
3to1_yz.gif
|
Stable 3:1 filament: surface density |
f3to1.gif
|
Internal dynamics of a stable 6:1 filament (xy-plane) |
6to1_xy.gif
|
6:1 stable filament (yz-plane) |
6to1_yz.gif
|
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Clemens: Wir sind nicht allein |
leben.pdf
|