HSC 2430

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0.19 UTI
0.0
CN
0.47
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.47 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2430 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the age 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)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 168.097 -65.207 0.431 -5.905 2.09 –
Hunt & Reffert 2024 168.177 -65.198 0.426 -5.909 2.074 –
Cavallo et al. 2024 168.106 -65.209 0.428 – – –
Hunt & Reffert 2023 168.177 -65.198 0.426 -5.909 2.074 –

💡 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– 2.17 1.635 0.77 85 -0.730 79 – –
Hunt & Reffert 2024 – – – – – 79(1) – –
Cavallo et al. 2024 2.16 1.60 – 17 -0.730 – – –
Hunt & Reffert 2023 2.18 1.67 0.77 153 – – – –

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

Visualization

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