HSC 2961

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0.49 UTI
0.45
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 7.7 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2961 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below 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 object shares a significant percentage of members with a later reported entry. See table with shared members information.

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– 267.443 -32.962 0.663 1.88 -1.798 -21.43
Hunt & Reffert 2024 267.432 -32.977 0.66 1.879 -1.776 -16.276
Cavallo et al. 2024 267.44 -32.928 0.662 – – –
Hunt & Reffert 2023 267.432 -32.977 0.66 1.879 -1.776 -16.276

💡 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– 1.275 2.965 2.45 44 -0.340 515 – –
Hunt & Reffert 2024 – – – – – 515(1) – –
Cavallo et al. 2024 1.11 2.98 – 68 -0.340 – – –
Hunt & Reffert 2023 1.44 2.95 2.45 21 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3015 57.8 267.44 -32.96 0.67 1.88 -1.81 -21.43 0.0

💡 Note: The % column shows the percentage of members that HSC 2961 shares with each listed object.

Visualization

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