HSC 2294

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0.09 UTI
0.31
CN
0.7
Cdens
0.25
CC3
0.25
Clit
0.26
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.7 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.26 Possibly duplicate

Overview

â„šī¸
HSC 2294 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 147.157 -58.669 0.214 -5.2 3.593 21.473
Hu & Soubiran 2025 147.136 -58.672 – – – –
Hunt & Reffert 2024 147.17 -58.668 0.212 -5.149 3.605 26.045
Cavallo et al. 2024 147.136 -58.672 0.21 – – –
Hunt & Reffert 2023 147.17 -58.668 0.212 -5.149 3.605 26.045

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 452* – –
Cavallo et al. 2024 3.37 1.79 – 661 0.460 – – –
Hunt & Reffert 2023 4.22 2.21 2.19 239 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3358 100.0 147.15 -58.67 0.22 -5.21 3.59 21.47 0.02
CWWDL 208 74.2 147.15 -58.67 0.23 -5.24 3.59 22.65 0.33

💡 Note: The % column shows the percentage of members that HSC 2294 shares with each listed object.

Visualization

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