HSC 1884

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0.15 UTI
0.26
CN
0.13
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1884 is a poorly populated, very 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-poor, 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.

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 117.184 -19.651 0.27 -2.224 2.406 –
Hunt & Reffert 2024 117.183 -19.629 0.278 -2.208 2.411 –
Cavallo et al. 2024 117.201 -19.651 0.28 – – –
Hunt & Reffert 2023 117.183 -19.629 0.278 -2.208 2.411 –

💡 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– 3.3 1.025 1.34 152 -0.530 181 – –
Hunt & Reffert 2024 – – – – – 181(1) – –
Cavallo et al. 2024 2.96 1.37 – 78 -0.530 – – –
Hunt & Reffert 2023 3.64 0.68 1.34 225 – – – –

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

Visualization

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