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tests:collision:mock_data [2016/12/16 14:33] – v.henault-brunettests:collision:mock_data [2022/10/24 12:27] (current) – external edit 127.0.0.1
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-[[:tests:collision:mock_data:Challenge_4|Challenge 4]]: Comparison of mass modelling methods using N-body model of M4.+[[:tests:collision:mock_data:Challenge_2|Challenge 2]]: Multi-mass clusters, no stellar evolution
  
-[[:tests:collision:mock_data: Challenge_2|Challenge 2]]: Multi-mass clusters, no stellar evolution +[[:tests:collision:mock_data:Challenge_3|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}} +
- +
- +
- +
-The definition of the stellar types (KSTAR) used in the ''NBODY6'' snapshots can be found in the [[:tests:collision:appendix|Appendix]].+
  
 +[[:tests:collision:mock_data:Challenge_4|Challenge 4]]: Comparison of mass modelling methods using N-body model of M4.
  
  
-===== Appendix =====+The definition of the stellar types (KSTAR) used in the ''NBODY6'' snapshots can be found in the [[:tests:collision:mock_data:appendix|Appendix]].
  
-==== Stellar types in ''NBODY'' ==== 
  
-There 23 possible stellar types (KSTAR) in ''NBODY'' 
  
-       0       Low main sequence (M < 0.7). 
-       1       Main sequence. 
-       2       Hertzsprung gap (HG). 
-       3       Red giant. 
-       4       Core Helium burning. 
-       5       First AGB. 
-       6       Second AGB. 
-       7       Helium main sequence. 
-       8       Helium HG. 
-       9       Helium GB. 
-      10       Helium white dwarf. 
-      11       Carbon-Oxygen white dwarf. 
-      12       Oxygen-Neon white dwarf. 
-      13       Neutron star. 
-      14       Black hole. 
-      15       Massless supernova remnant. 
-      19       Circularizing binary (c.m. value). 
-      20       Circularized binary. 
-      21       First Roche stage (inactive). 
-      22       Second Roche stage. 
tests/collision/mock_data.1481898797.txt.gz · Last modified: 2022/10/24 12:26 (external edit)