UPK 156

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0.21 UTI
0.0
CN
0.16
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 18.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UPK 156 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied 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.

Close Low extinction Near-solar metallicity Intermediate age

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 – 328.404 51.805 1.06 -0.328 -1.899 -18.175
Hunt & Reffert 2024 328.4 51.958 1.065 -0.321 -1.858 -15.565
Cavallo et al. 2024 328.434 51.907 1.067 – – –
Hunt & Reffert 2023 328.4 51.958 1.065 -0.321 -1.858 -15.565
Sim et al. 2019 328.463 51.865 – -0.32 -1.91 –

💡 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
Hunt & Reffert 2024 – – – – – 51* – –
Cavallo et al. 2024 0.95 1.01 – 245 0.120 – – –
Hunt & Reffert 2023 0.90 0.81 0.32 195 – – – –
Sim et al. 2019 0.90 – – 79 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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