HSC 1331

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0.18 UTI
0.0
CN
0.26
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.26 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1331 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 76.71 35.39 1.065 -0.231 -2.99 8.479
Zhang et al. 2024 76.847 35.21 – – – –
Cavallo et al. 2024 76.653 35.369 1.06 – – –
Hunt & Reffert 2023 76.847 35.21 1.062 -0.221 -2.99 2.582

💡 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
Zhang et al. 2024 – – – – 0.022* – – –
Cavallo et al. 2024 0.97 1.60 – 427 0.170 – – –
Hunt & Reffert 2023 0.90 1.46 0.60 92 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4127 76.0 76.56 35.46 1.06 -0.2 -2.97 8.48 0.04

💡 Note: The % column shows the percentage of members that HSC 1331 shares with each listed object.

Visualization

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