HSC 2972

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0.33 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 6.7 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2972 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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– 265.773 -31.041 0.782 -0.28 -3.17 –
Hunt & Reffert 2024 265.775 -31.043 0.775 -0.25 -3.18 –
Cavallo et al. 2024 265.764 -31.066 0.775 – – –
Hunt & Reffert 2023 265.775 -31.043 0.775 -0.25 -3.18 –

💡 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– 1.665 4.225 2.51 36 -1.460 300 – –
Hunt & Reffert 2024 – – – – – 300(1) – –
Cavallo et al. 2024 2.13 4.38 – 42 -1.460 – – –
Hunt & Reffert 2023 1.20 4.07 2.51 30 – – – –

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

Visualization

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