OC 0127

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0.20 UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.25
Clit
0.88
Cdup
Radius (P>50% members) 8.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.88 Very likely unique

Overview

â„šī¸
OC 0127 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Massive Metal-rich Young

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 – 304.295 42.801 0.501 -3.035 -4.572 –
Hunt & Reffert 2024 304.43 42.714 0.487 -3.011 -4.582 -24.428
Cavallo et al. 2024 304.445 42.775 0.494 – – –
Hunt & Reffert 2023 304.43 42.714 0.487 -3.011 -4.582 -24.428
Hao et al. 2022 304.172 42.856 0.49 -2.939 -4.535 –

💡 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 – – – – – 1044* – –
Cavallo et al. 2024 2.04 2.40 – 69 0.720 – – –
Hunt & Reffert 2023 1.88 2.55 2.50 30 – – – –
Hao et al. 2022 – 4.39 – 79 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0232 12.0 304.52 42.64 0.4 -2.92 -4.66 – 0.14

💡 Note: The % column shows the percentage of members that OC 0127 shares with each listed object.

Visualization

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