HSC 1653

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0.37 UTI
0.3
CN
0.53
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.53 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1653 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 79.452 -8.456 3.201 0.385 -0.724 18.042
Zhang et al. 2024 79.36 -8.504 – – – –
Cavallo et al. 2024 79.373 -8.396 3.21 – – –
Hunt & Reffert 2023 79.36 -8.504 3.212 0.361 -0.766 10.138

💡 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– 0.31 0.83 0.96 12 0.142 – – –
Zhang et al. 2024 – – – – 0.125(1) – – –
Cavallo et al. 2024 0.31 0.83 – 14 0.160 – – –
Hunt & Reffert 2023 0.31 0.83 0.96 10 – – – –

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

Visualization

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