HSC 1330

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0.10 UTI
0.0
CN
0.12
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 30.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1330 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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 Low 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 – 85.942 42.151 1.623 0.03 -2.704 -6.599
Zhang et al. 2024 86.645 40.405 – – – –
Cavallo et al. 2024 86.542 40.666 1.637 – – –
Hunt & Reffert 2023 86.645 40.405 1.641 0.063 -2.741 -12.414

💡 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 – – – – -0.085* – – –
Cavallo et al. 2024 0.63 0.83 – 178 0.000 – – –
Hunt & Reffert 2023 0.59 0.42 0.62 239 – – – –

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

Visualization

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