Snapshots ouputs
Here, we provide a summary of the quantities written in the snapshots, in addition to positions, velocities, masses, smoothing lengths and particle IDs.
The tracer outputs are summarised on the Particle tracers page.
Sink particles
Name |
Description |
Units |
Comments |
|---|---|---|---|
|
Number of merger events with other sinks
|
[-] |
|
|
Number of gas particles accreted
|
[-] |
|
|
Target mass required 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 this sink
|
[-] |
|
|
Total angular momentum of accreted
material
|
[U_M U_L^2 U_T^{-1}] |
|
|
Mass fraction of each tracked metal
element
|
[-] |
Only in GEAR chemistry module.
Array of length
N (number of elements),set at compile time via
--with-chemistry=GEAR_N. |
|
Scale factor at the time of sink creation
|
[-] |
Only used in cosmological runs.
|
|
Time when the sink was created
|
[U_T] |
Only used in non-cosmological runs.
|
|
Physical densities at the time of birth
|
[U_M U_L^{-3}] |
Stored at birth time/redshift.
|
|
Temperatures at the time of birth
|
[U_K] |
Stored at birth time/redshift.
|
|
Physical instantaneous accretion rates
|
[U_M U_T^{-1}] |
At the current step
|
|
Star formation rates of the particles
|
[U_M U_T^{-1}] |
If negative, stores last time/scale-factor
at which gas was star-forming.
|
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 birth time
|
[U_M] |
SF and sinks modules
|
|
ID of the progenitor sinks or gas
particles
|
[-] |
SF and sinks modules
|
|
Gas density at star formation
|
[U_M U_L^{-3}] |
Only in SF module
|
|
Gas temperature at star formation
|
[K] |
Only in SF module
|
|
Gravitational potential of the star
|
[U_L^2 U_T^{-2}] |
|
|
Type of the stellar particle:
|
[-] |
0: (discrete) single star
1: continuous IMF part star
2: single population star
The last type corresponds to legacy IMF stars.
|
|
Mass fraction of each metal element
|
[-] |
Only in GEAR chemistry module.
Array of length
N (number of elements),set at compile time by
--with-chemistry=GEAR_N. |
Gas particles
Since hydro scheme writes its own set of outputs, we only provide the outputs that GEAR writes for gas particles.
Name |
Description |
Units |
Comments |
|---|---|---|---|
|
Mass fraction of each metal element
smoothed over the SPH kernel
|
[-] |
Only in GEAR chemistry module.
Array of length
N, set at compile time by--with-chemistry=GEAR_N |
|
Raw (non-smoothed) mass fraction of
each metal element
|
[-] |
Only in GEAR chemistry module.
Same layout as above.
|
|
Mass fraction of neutral H (\(\mathrm{H}\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Mass fraction of ionized H (\(\mathrm{H}^+\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Mass fraction of neutral He (\(\mathrm{He}\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Mass fraction of singly ionized He (\(\mathrm{He}^+\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Mass fraction of doubly ionized He
(\(\mathrm{He}^{++}\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Free electron mass fraction (\(\mathrm{e}^-\))
|
[-] |
Only if
GRACKLE_1 to 3 |
|
Mass fraction of \(\mathrm{H}^-\)
|
[-] |
Only if
GRACKLE_2 or 3 |
|
Mass fraction of neutral \(\mathrm{H}_2\)
|
[-] |
Only if
GRACKLE_2 or 3 |
|
Mass fraction of ionized \(\mathrm{H}_2^+\)
|
[-] |
Only if
GRACKLE_2 or 3 |
|
Mass fraction of neutral D (\(\mathrm{D}\))
|
[-] |
Only if
GRACKLE_3 |
|
Mass fraction of ionized D (\(\mathrm{D}^+\))
|
[-] |
Only if
GRACKLE_3 |
|
Mass fraction of \(\mathrm{HD}\)
|
[-] |
Only if
GRACKLE_3 |