Snapshots ouputs
Here, we provide a summary of the quantities written in the snapshots, in addition to positions, velocities, masses and particle IDs.
Sink particles
Name |
Description |
Units |
Comments |
---|---|---|---|
|
Number of sink merger events
|
[-] |
|
|
Number of gas swallowed
|
[-] |
|
|
Sink target mass to spawn the
next star particle
|
[U_M] |
You can use it to determine if the target mass
is so huge that the sink’s mass cannot spawn
such a star. Such rare behaviour may bias the
IMF towards high masses.
|
|
Number of stars created by the
the sink particles
|
[-] |
|
|
Total angular momentum swallowed
by the sink particles
|
|
|
|
Mass fraction of each metal
element
|
[-] |
Array of length
N for each particles. Thenumber of elements
N is determined atcompile time by
--with-chemistry=GEAR_N . |
Stars
Name |
Description |
Units |
Comments |
---|---|---|---|
|
Scale-factors when the stars were
born
|
[-] |
Only used in cosmological runs. |
|
Time when the stars were
born
|
[U_T] |
Only used in non-cosmological runs. |
|
Masses of the stars at brith time
|
[U_M] |
|
|
ID of the progenitor sinks
|
[-] |
|
|
Type of the stellar particle:
0: (discrete) single star
1: continuous IMF part star
2: single population star
|
[-] |
The last type correspond to star particles in
the previous model, i.e. representing the full
IMF
|