HSC 243

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0.32 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.57
Cdup
Stellar density (N50/rad) 11.2 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.57 Likely unique

Overview

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HSC 243 is a rich, 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, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P228, along with OC_0043.

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 279.081 -6.74 0.354 -0.139 -2.245 39.939
Hunt & Reffert 2024 279.073 -6.763 0.354 -0.136 -2.243 95.009
Cavallo et al. 2024 279.084 -6.726 0.355 – – –
Hunt & Reffert 2023 279.073 -6.763 0.354 -0.136 -2.243 95.009

💡 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] Bfrac BSS
UCC 99999– 2.775 4.525 3.04 10 0.430 2594 – –
Hunt & Reffert 2024 – – – – – 2594(1) – –
Cavallo et al. 2024 2.96 4.55 – 7 0.430 – – –
Hunt & Reffert 2023 2.59 4.50 3.04 12 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
G3CC 58 42.5 279.08 -6.68 0.35 -0.14 -2.23 17.9 0.51
OC 0045 28.8 279.08 -6.67 0.35 -0.15 -2.2 – 0.02
Ryu 865 3.4 279.19 -6.78 0.35 -0.27 -2.24 – 0.22

💡 Note: The % column shows the percentage of members that HSC 243 shares with each listed object.

Visualization

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