Challenge 3. Clusters in tidal fields with stellar evolution []

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====== Challenge 3. Clusters in tidal fields with stellar evolution ======
(Simulations ran and kindly made available by Holger Baumgardt)\\

Here we consider 2 clusters which are slightly more realistic:

  - IC: King (1966) W_0 = 5 model, N = 131072, Kroupa (2001) mass function between 0.1-15 Msun (no black-holes).
  - No primordial binaries, no central black hole, circular orbit in logarithmic halo with V = 220 km/s.
  - Z = 0.001
  - Stellar evolution and mass-loss according to Hurley et al. (2000, 2002)
  - Two Galactocentric radii: 8.5 kpc and 15 kpc.


Below are 2 snapshots at an age of roughly 10 Myr, 100 Myr, 1Gyr and 12 Gyr. The columns are the same as in Challenge 2.

  - {{:data:W05_N131K_RG8.5_FEH-0.0_T10.gz}} UPDATED! Thursday August 22
  - {{:data:W05_N131K_RG8.5_FEH-0.0_T100.gz}} UPDATED! Thursday August 22
  - {{:data:W05_N131K_RG8.5_FEH-0.0_T1000.gz}} UPDATED! Thursday August 22
  - {{:W05_N131K_RG8.5_FEH-0.0_T12000.gz}}
  - {{:data:W05-N131K_RG15_FEH-0.0.T10.gz}} NEW! Tuesday August 20
  - {{:data:W05-N131K_RG15_FEH-0.0.T100.gz}} NEW! Tuesday August 20
  - {{:data:W05-N131K_RG15_FEH-0.0.T1000.gz}} NEW! Tuesday August 20
  - {{:W05_N131K_RG15_FEH-0.0_T12000.gz}}

Final list of snapshots used in Sollima et al. in prep, columns are:

^ $m$    ^ $X$ ^ $Y$ ^ $Z$ ^ $V_x$ ^ $V_y$ ^ $V_z$ ^ kstar ^ logL ^ logTeff ^
| [Msun] |[pc] |[pc] |[pc] | [km/s |[km/s] |[km/s] |       |      |         |

  - {{:data:W5rh11.5R8.5-t0.gz}}
  - {{:data:W5rh11.5R8.5-t10024.05.gz}}
  - {{:data:W5rh11.5R8.5-t1019.394.gz}}
  - {{:data:W5rh11.5R8.5-t11009.46.gz}}
  - {{:data:W5rh11.5R8.5-t2004.809.gz}}
  - {{:data:W5rh11.5R8.5-t3024.204.gz}}
  - {{:data:W5rh11.5R8.5-t4009.618.gz}}
  - {{:data:W5rh11.5R8.5-t5029.013.gz}}
  - {{:data:W5rh11.5R8.5-t6014.427.gz}}
  - {{:data:W5rh11.5R8.5-t7033.822.gz}}
  - {{:data:W5rh11.5R8.5-t8019.236.gz}}
  - {{:data:W5rh11.5R8.5-t9004.651.gz}}
  - {{:data:W5rh1R8.5-t0.gz}}
  - {{:data:W5rh1R8.5-t10020.gz}}
  - {{:data:W5rh1R8.5-t1020.gz}}
  - {{:data:W5rh1R8.5-t11010.gz}}
  - {{:data:W5rh1R8.5-t120.gz}}
  - {{:data:W5rh1R8.5-t12000.gz}}
  - {{:data:W5rh1R8.5-t13020.gz}}
  - {{:data:W5rh1R8.5-t2010.gz}}
  - {{:data:W5rh1R8.5-t210.gz}}
  - {{:data:W5rh1R8.5-t30.gz}}
  - {{:data:W5rh1R8.5-t300.gz}}
  - {{:data:W5rh1R8.5-t3000.gz}}
  - {{:data:W5rh1R8.5-t4020.gz}}
  - {{:data:W5rh1R8.5-t420.gz}}
  - {{:data:W5rh1R8.5-t5010.gz}}
  - {{:data:W5rh1R8.5-t510.gz}}
  - {{:data:W5rh1R8.5-t60.gz}}
  - {{:data:W5rh1R8.5-t6000.gz}}
  - {{:data:W5rh1R8.5-t7020.gz}}
  - {{:data:W5rh1R8.5-t8010.gz}}
  - {{:data:W5rh1R8.5-t90.gz}}
  - {{:data:W5rh1R8.5-t9000.gz}}