HSC 385

Click to load Aladin Lite
0.18 UTI
0.0
CN
0.66
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.66 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 385 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, 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.

Palma et al. (2025)
Classified as optical pair P336, along with CWNU_1893.

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 288.391 10.328 0.452 -1.804 -3.145 29.237
Hunt & Reffert 2024 288.39 10.333 0.454 -1.766 -3.144 -40.315
Cavallo et al. 2024 288.381 10.324 0.456 – – –
Hunt & Reffert 2023 288.39 10.333 0.454 -1.766 -3.144 -40.315

💡 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– 2.015 4.025 2.07 29 0.570 211 – –
Hunt & Reffert 2024 – – – – – 211(1) – –
Cavallo et al. 2024 1.98 3.65 – 32 0.570 – – –
Hunt & Reffert 2023 2.05 4.40 2.07 26 – – – –

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

Visualization

â„šī¸