HSC 1484

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0.05 UTI
0.0
CN
0.1
Cdens
0.62
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

â„šī¸
HSC 1484 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

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– 94.551 24.829 0.172 0.211 -0.724 –
Hunt & Reffert 2024 94.564 24.829 0.164 0.247 -0.738 –
Cavallo et al. 2024 94.56 24.776 0.163 – – –
Hunt & Reffert 2023 94.564 24.829 0.164 0.247 -0.738 –

💡 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– 5.145 1.675 1.56 48 0.640 249 – –
Hunt & Reffert 2024 – – – – – 249(1) – –
Cavallo et al. 2024 4.94 1.56 – 56 0.640 – – –
Hunt & Reffert 2023 5.35 1.79 1.56 39 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Koposov 62 64.0 94.53 24.76 0.17 0.24 -0.74 – 0.36

💡 Note: The % column shows the percentage of members that HSC 1484 shares with each listed object.

Visualization

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