HSC 1734

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0.12 UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1734 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 109.125 -4.561 0.363 -1.446 -0.142 58.67
Hunt & Reffert 2024 109.071 -4.423 0.362 -1.437 -0.119 60.697
Cavallo et al. 2024 109.121 -4.519 0.362 – – –
Hunt & Reffert 2023 109.071 -4.423 0.362 -1.437 -0.119 60.697

💡 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– 2.6 0.495 0.73 285 0.040 79 – –
Hunt & Reffert 2024 – – – – – 79(1) – –
Cavallo et al. 2024 2.45 0.69 – 269 0.040 – – –
Hunt & Reffert 2023 2.75 0.30 0.73 301 – – – –

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

Visualization

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