Run 4
T/Myr |
Ns + Nb |
Mtot/Msun |
Rh/pc |
0 |
16384 |
10174 |
5.414 |
500 |
14872 |
7214 |
6.925 |
1000 |
13198 |
6172 |
7.172 |
1500 |
11523 |
5354 |
7.117 |
2000 |
9908 |
4683 |
6.914 |
2500 |
8434 |
4075 |
6.508 |
3000 |
6871 |
3458 |
6.159 |
3500 |
5520 |
2888 |
5.537 |
4000 |
4401 |
2428 |
5.089 |
4500 |
3511 |
2026 |
4.307 |
5000 |
2605 |
1602 |
3.582 |
5500 |
1955 |
1265 |
3.065 |
5638.77 |
1784 |
1175 |
3.133 RUN STOPPED |
Figures
-
radii
(for core and 50 and 75% Lagrangian radii)against time.
-
mass
function at t = 0, 2.49, 3.56 and 5.64 Gyr
-
XY
position relative to original position
-
XZ
position relative to original position (only until about 3.5Gyr)
-
mass
(solid) and number of stars (dashed) as a function of time
-
number
of stars of different types as a function of time. Key:
-
Solid: all
-
upper dash: main-sequence
-
lower dash: giants
-
dotted: white dwarfs
-
dash-dot: neutron star+ black hole
Note: there is some doubt about either the implementation of the tide
in this run, or whether stellar evolution was included.