HSC 2576

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0.27 UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.55
Cdup
Stellar density (N50/rad) 9.1 [N/pc2]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.55 Likely unique

Overview

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HSC 2576 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate 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)
Part of multiple system G160, along with HSC_2569 and NGC_5045.

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– 199.65 -62.571 0.487 -4.3 -1.74 -29.392
Hunt & Reffert 2024 199.678 -62.525 0.485 -4.38 -1.742 -28.043
Cavallo et al. 2024 199.427 -62.599 0.484 – – –
Hunt & Reffert 2023 199.678 -62.525 0.485 -4.38 -1.742 -28.043

💡 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– 1.76 1.6 2.38 11 -0.400 1033 – –
Hunt & Reffert 2024 – – – – – 1033(1) – –
Cavallo et al. 2024 1.59 1.60 – 12 -0.400 – – –
Hunt & Reffert 2023 1.93 1.60 2.38 10 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 526 44.9 199.68 -62.54 0.49 -4.16 -1.81 -37.02 0.45
DBSB 85 9.2 199.65 -62.67 0.38 -4.5 -1.88 -38.19 0.3
VVV 024 2.0 199.65 -62.74 0.38 -4.89 -1.58 – 0.05

💡 Note: The % column shows the percentage of members that HSC 2576 shares with each listed object.

Visualization

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