Data for the paper: Multiple Stellar Populations in MOCCA Models – Transient Spatial Over-Concentration of Pristine RGB Stars

This dataset contains MOCCA simulation data for a globular cluster model used in the publication:"Multiple stellar populations in MOCCA globular cluster models: Transient spatial over-concentration of pristine red giant stars driven by strong dynamical encounters." Preprint for the paper is available at: https://arxiv.org/abs/2502.17162

The simulation was performed using the MOCCA code version described in Giersz et al. (2024):https://arxiv.org/abs/2411.06421

Included Files

This dataset contains three files from the MOCCA simulation:

mocca.ini – The input configuration file used for the MOCCA simulation.

system.dat – A file containing detailed record of the cluster evolution, storing over 500 parameters related to:

Global cluster properties

Stellar and binary system properties

Technical parameters

Dynamical interactionsThe first 2450 lines in this file contain header descriptions for all columns.Please Note: Changes in the etot column during the first 100 Myr are due to the gradual accretion of mass onto gas particles in the initial model. This process leads to a time-dependent variation in total energy, which should be considered when analyzing energy evolution.

snap13.dat – The non-projected 13 Gyr snapshot of the simulation, containing 35 columns (described below).

Column Descriptions for snap13.dat (13 Gyr Snapshot)

im – Star/binary name (inames/inameb)

r – Position in the cluster (pc)

vr – Radial velocity (km/s)

vt – Tangential velocity (km/s)

u – Potential energy [MC units]

ikb – Binary type (0 = single, 1 = binary, 2 = semi-detached binary)

a – Semi-major axis of a binary (solar radii, R☉), 0.0 for single stars

e – Eccentricity of the binary, 0.0 for single stars

ik1 – SSE/BSE stellar type of the first component (see table below)

ik2 – SSE/BSE stellar type of the second component

sm1 – Mass of the first component (solar mass, M☉)

sm2 – Mass of the second component (solar mass, M☉), 0.0 for single stars

popId1 – Population ID of the first component (1 = pristine, 2 = enriched, >=100 for mixed pop)

popId2 – Population ID of the second component

timenr – Timestep (integer)

idd1 – Star/binary ID for the first component

idd2 – Star/binary ID for the second component

lum1 – Luminosity of the first component (bolometric solar luminosity, L☉)

lum2 – Luminosity of the second component (bolometric solar luminosity, L☉)

rad1 – Radius of the first component (solar radii, R☉)

rad2 – Radius of the second component (solar radii, R☉)

hist1 – Compact history of the first star (dynamical events, mergers, etc.)

hist2 – Compact history of the second star

spin1 – Spin of the first component (SSE/BSE)

spin2 – Spin of the second component (SSE/BSE)

mu1 – U-band magnitude for the first component

mu2 – U-band magnitude for the second component

mv1 – V-band magnitude for the first component

mv2 – V-band magnitude for the second component

mb1 – B-band magnitude for the first component

mb2 – B-band magnitude for the second component

mi1 – I-band magnitude for the first component

mi2 – I-band magnitude for the second component

mtr1 – Mass transfer rate of the first component (solar mass per year, M☉/yr)

mtr2 – Mass transfer rate of the second component (solar mass per year, M☉/yr)

The compact history columns (hist1, hist2) above encode the short history of the events with the star

0000000000000000001 - had dynamical collision (inter-coll)

0000000000000000010 - had binary merger (stellar evolution)

0000000000000000100 - had mass transfer event in binary evolution (increased the mass)

0000000000000001000 - had interaction (bin-bin, or bin-sin)

0000000000000010000 - had exchange in interaction

0000000000000100000 - went to a binary (inter-binform)

0000000000001000000 - went to single (dissolution in stellar evolution)

0000000000010000000 - went to single (dissolution in interaction)

0000000000100000000 - separation changed by 1% (in interaction)

0000000001000000000 - separation changed by 10% (in interaction)

0000000010000000000 - eccentricity changed by 1% (in interaction)

0000000100000000000 - eccentricity changed by 10% (in interaction)

0000001000000000000 - dissolution in bin-sin interaction

0000010000000000000 - dissolution in bin-bin interaction

0000100000000000000 - dissolution in binary evolution

0001000000000000000 - exchange in bin-sin interaction

0010000000000000000 - exchange in bin-bin interaction

0100000000000000000 - dynamical collision in bin-sin

1000000000000000000 - dynamical collision in bin-bin (or hierarchical)E.g. if the star had two dynamical collisions and 5 mass transfer events in binary evolution then it has hist column value of: 0000000052

The values in ik1 and ik2 correspond to SSE/BSE stellar types from Hurley et al. (2000; 2002):

0 - Fully convective low-mass MS star (M < 0.7 M☉)1 - Main Sequence star (M > 0.7 M☉)2 - Hertzsprung Gap (subgiant star)3 - First Giant Branch4 - Core Helium Burning5 - First Asymptotic Giant Branch6 - Second Asymptotic Giant Branch7 - Main Sequence Naked Helium star8 - Hertzsprung Gap Naked Helium star9 - Giant Branch Naked Helium star10 - Helium White Dwarf11 - Carbon/Oxygen White Dwarf12 - Oxygen/Neon White Dwarf13 - Neutron Star14 - Black Hole

If you have any questions about the data or require more extensive data then please feel free to contact us.