HSC 1721

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0.16 UTI
0.0
CN
0.26
Cdens
0.25
CC3
0.25
Clit
0.8
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.26 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.8 Very likely unique

Overview

â„šī¸
HSC 1721 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.8) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Liu et al. (2025)
Classified as primordial binary cluster 204 along with HSC_1723, and as tidal capture (resonant trapping binary) 282 along with NGC_2311, and of multiple system 58 along with HSC_1722, HSC_1723 and NGC_2311.

Palma et al. (2025)
Part of multiple system G128, along with HSC_1723 and HSC_1722.

Cavallo et al. (2024)
Silver 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– 104.967 -4.518 0.446 -1.89 0.601 –
Liu et al. 2025 104.98 -4.5 0.44 -1.89 0.57 –
Hunt & Reffert 2024 104.983 -4.501 0.444 -1.886 0.568 –
Cavallo et al. 2024 104.995 -4.505 0.444 – – –
Hunt & Reffert 2023 104.983 -4.501 0.444 -1.886 0.568 –

💡 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– 2.36 1.28 1.05 24 -0.210 117 – –
Liu et al. 2025 3.89 0.48 – 13 – – – –
Hunt & Reffert 2024 – – – – – 117(1) – –
Cavallo et al. 2024 2.36 1.28 – 24 -0.210 – – –
Hunt & Reffert 2023 2.11 1.47 1.05 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Sh2 287C 20.0 104.85 -4.7 0.45 -1.61 0.76 48.19 0.09

💡 Note: The % column shows the percentage of members that HSC 1721 shares with each listed object.

Visualization

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