OC 0257

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0.15 UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 22.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0257 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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 Moderate 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 – 46.058 59.297 1.192 -0.182 -1.433 -14.009
Hunt & Reffert 2024 46.16 59.27 1.197 -0.113 -1.429 -13.125
Cavallo et al. 2024 46.06 59.257 1.193 – – –
Hunt & Reffert 2023 46.16 59.27 1.197 -0.113 -1.429 -13.125
Hao et al. 2022 46.179 59.255 1.186 -0.267 -1.278 –

💡 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 – – – – – 79* – –
Cavallo et al. 2024 0.82 1.34 – 355 0.230 – – –
Hunt & Reffert 2023 0.82 1.61 0.79 95 – – – –
Hao et al. 2022 – 3.72 – 316 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1154 84.0 46.04 59.25 1.2 -0.18 -1.45 -14.01 0.01

💡 Note: The % column shows the percentage of members that OC 0257 shares with each listed object.

Visualization

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