HSC 1239

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0.13 UTI
0.0
CN
0.27
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 31.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.27 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1239 is a sparse, loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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.

Very close Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Wood 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 – 57.249 39.125 2.328 8.192 -7.652 3.434
Cavallo et al. 2024 56.992 39.282 2.319 – – –
Hunt & Reffert 2023 57.401 38.957 2.311 8.153 -7.636 -7.349

💡 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] Bfr BSS
Cavallo et al. 2024 0.55 0.70 – 5012 0.400 – – –
Hunt & Reffert 2023 0.40 1.57 1.04 6 – – – –

Visualization

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