HSC 1328

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0.13 UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1328 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young 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.

Very distant Moderate extinction Metal-rich Young

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 – 82.69 38.607 0.18 0.056 -0.857 -31.455
Hunt & Reffert 2024 82.695 38.6 0.179 0.044 -0.855 –
Cavallo et al. 2024 82.66 38.649 0.182 – – –
Hunt & Reffert 2023 82.695 38.6 0.179 0.044 -0.855 –

💡 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
Hunt & Reffert 2024 – – – – – 452* – –
Cavallo et al. 2024 4.70 2.46 – 63 0.540 – – –
Hunt & Reffert 2023 5.50 2.58 0.47 15 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3573 100.0 82.67 38.63 0.17 0.06 -0.86 -39.38 0.11

💡 Note: The % column shows the percentage of members that HSC 1328 shares with each listed object.

Visualization

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