HSC 108

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0.21 UTI
0.66
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.4
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.66 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.4 Possibly duplicate

Overview

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HSC 108 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~3.29 kpc) differs significantly from the median photometric distance (~2.49 kpc).

Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 271.324 -22.935 0.304 -0.057 -1.416 16.268
Hunt & Reffert 2024 271.327 -22.928 0.31 -0.075 -1.448 16.251
Cavallo et al. 2024 271.332 -22.942 0.309 – – –
Hunt & Reffert 2023 271.327 -22.928 0.31 -0.075 -1.448 16.251

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 1548* – –
Cavallo et al. 2024 2.22 3.23 – 288 0.340 – – –
Hunt & Reffert 2023 2.76 3.29 2.61 106 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1685 60.5 271.35 -22.94 0.3 -0.1 -1.47 15.66 0.45
CWNU 3539 42.0 271.32 -22.95 0.29 -0.05 -1.37 37.42 0.0

💡 Note: The % column shows the percentage of members that HSC 108 shares with each listed object.

Visualization

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