HSC 262

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0.36 UTI
0.5
CN
0.57
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.8 [N/pc2]
  • CN 0.5 Moderately populated
  • Cdens 0.57 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 262 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, very 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)
Bronze 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– 280.25 -5.648 0.22 -1.229 -3.12 52.828
Hunt & Reffert 2024 280.25 -5.645 0.217 -1.197 -3.1 52.871
Cavallo et al. 2024 280.266 -5.651 0.219 – – –
Hunt & Reffert 2023 280.25 -5.645 0.217 -1.197 -3.1 52.871

💡 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– 3.88 4.32 2.9 10 -1.100 990 – –
Hunt & Reffert 2024 – – – – – 990(1) – –
Cavallo et al. 2024 3.77 5.13 – 3 -1.100 – – –
Hunt & Reffert 2023 3.99 3.51 2.90 16 – – – –

(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 4043 64.7 280.25 -5.63 0.24 -1.25 -3.15 52.19 0.06

💡 Note: The % column shows the percentage of members that HSC 262 shares with each listed object.

Visualization

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