HSC 1312

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0.39 UTI
0.26
CN
0.45
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.2 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1312 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above 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.

Note: This object shares a large 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– 81.294 40.24 0.214 0.455 -0.566 –
Zhang et al. 2024 81.305 40.246 – – – –
Hunt & Reffert 2024 81.305 40.246 0.217 0.444 -0.568 8.43
Cavallo et al. 2024 81.299 40.235 0.215 – – –
Hunt & Reffert 2023 81.305 40.246 0.217 0.444 -0.568 8.43

💡 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– 4.09 1.925 1.31 235 0.046 336 – –
Zhang et al. 2024 – – – – -0.327(1) – – –
Hunt & Reffert 2024 – – – – – 336(1) – –
Cavallo et al. 2024 4.06 1.91 – 245 0.420 – – –
Hunt & Reffert 2023 4.12 1.94 1.31 225 – – – –

(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 3058 96.2 81.3 40.23 0.21 0.45 -0.57 – 0.02

💡 Note: The % column shows the percentage of members that HSC 1312 shares with each listed object.

Visualization

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