HSC 2862

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0.43 UTI
0.76
CN
0.83
Cdens
1.0
CC3
0.0
Clit
0.83
Cdup
Stellar density (N50/rad) 4.1 [N/pc2]
  • CN 0.76 Rich
  • Cdens 0.83 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.83 Very likely unique

Overview

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HSC 2862 is a rich, dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very 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 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.

Palma et al. (2025)
Classified as optical pair P491, along with HSC_2868.

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– 258.434 -40.786 0.286 -1.522 -3.124 -35.448
Hunt & Reffert 2024 258.442 -40.788 0.295 -1.529 -3.114 29.528
Cavallo et al. 2024 258.357 -40.768 0.294 – – –
Hunt & Reffert 2023 258.442 -40.788 0.295 -1.529 -3.114 29.528

💡 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– 2.99 5.365 3.1 15 0.390 4559 – –
Hunt & Reffert 2024 – – – – – 4559(1) – –
Cavallo et al. 2024 2.86 5.16 – 8 0.390 – – –
Hunt & Reffert 2023 3.12 5.57 3.10 22 – – – –

(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 0676 16.7 258.2 -40.75 0.3 -1.54 -3.12 -6.02 0.23

💡 Note: The % column shows the percentage of members that HSC 2862 shares with each listed object.

Visualization

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