HSC 1323

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0.17 UTI
0.0
CN
0.12
Cdens
0.62
CC3
0.3
Clit
0.64
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 0.64 Likely unique

Overview

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HSC 1323 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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.

Liu et al. (2025)
Classified as primordial binary cluster 41 along with COIN-Gaia_16.

Palma et al. (2025)
Part of multiple system G112, along with HSC_1321 and COIN-Gaia_16.

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 99999– 79.389 37.855 0.64 0.986 -3.528 -19.407
Zhang et al. 2024 79.348 37.892 – – – –
Hunt & Reffert 2024 79.348 37.892 0.632 1.01 -3.544 -41.149
Cavallo et al. 2024 79.411 37.8 0.632 – – –
Hunt & Reffert 2023 79.348 37.892 0.632 1.01 -3.544 -41.149

💡 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– 1.58 0.4 1.26 35 -0.293 118 – –
Liu et al. 2025 2.18 0.26 – 21 – – – –
Zhang et al. 2024 – – – – -0.247(1) – – –
Hunt & Reffert 2024 – – – – – 118(1) – –
Cavallo et al. 2024 1.58 0.75 – 55 -0.340 – – –
Hunt & Reffert 2023 1.49 0.40 1.26 35 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0287 36.0 79.46 38.03 0.62 1.04 -3.6 -19.37 0.12
UBC 63 36.0 79.65 37.84 0.64 1.08 -3.55 -26.85 0.5

💡 Note: The % column shows the percentage of members that HSC 1323 shares with each listed object.

Visualization

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