HSC 689

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0.11 UTI
0.0
CN
0.28
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 689 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

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 99999– 321.469 42.515 1.584 2.62 -0.827 -19.204
Zhang et al. 2024 321.57 42.483 – – – –
Cavallo et al. 2024 321.554 42.541 1.583 – – –
Hunt & Reffert 2023 321.57 42.483 1.584 2.575 -0.978 -33.117

💡 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– 0.615 0.245 0.44 76 0.098 – – –
Zhang et al. 2024 – – – – 0.025(1) – – –
Cavallo et al. 2024 0.62 0.33 – 91 0.170 – – –
Hunt & Reffert 2023 0.61 0.16 0.44 61 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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