HSC 1886

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0.19 UTI
0.26
CN
0.42
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.42 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1886 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate 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.

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 99999– 115.664 -20.692 0.24 -1.676 2.543 –
Hunt & Reffert 2024 115.684 -20.733 0.22 -1.68 2.539 88.313
Cavallo et al. 2024 115.663 -20.694 0.226 – – –
Hunt & Reffert 2023 115.684 -20.733 0.22 -1.68 2.539 88.313

💡 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– 4.415 1.24 1.88 95 0.620 261 – –
Hunt & Reffert 2024 – – – – – 261(1) – –
Cavallo et al. 2024 5.22 1.25 – 50 0.620 – – –
Hunt & Reffert 2023 3.61 1.23 1.88 140 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3232 84.6 115.65 -20.68 0.24 -1.67 2.54 – 0.04

💡 Note: The % column shows the percentage of members that HSC 1886 shares with each listed object.

Visualization

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