HSC 1693

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0.18 UTI
0.27
CN
0.28
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.28 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1693 is a poorly populated, 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.525 -1.141 1.063 -1.417 -1.817 23.588
Zhang et al. 2024 104.439 -1.143 – – – –
Cavallo et al. 2024 104.622 -1.371 1.055 – – –
Hunt & Reffert 2023 104.439 -1.143 1.053 -1.445 -1.843 28.753

💡 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– 0.945 0.17 0.53 119 0.121 – – –
Zhang et al. 2024 – – – – -0.057(1) – – –
Cavallo et al. 2024 0.98 0.27 – 129 0.300 – – –
Hunt & Reffert 2023 0.91 0.07 0.53 109 – – – –

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

Visualization

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