OC 0668

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0.00 UTI
0.41
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0668 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Massive 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 – 251.043 -44.113 0.289 -2.498 -4.004 -54.568
Hunt & Reffert 2024 251.045 -44.113 0.297 -2.502 -3.969 -59.905
Cavallo et al. 2024 251.037 -44.122 0.296 – – –
Hunt & Reffert 2023 251.045 -44.113 0.297 -2.502 -3.969 -59.905
Hao et al. 2022 251.04 -44.105 0.332 -2.492 -3.977 –

💡 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 – – – – – 2855* – –
Cavallo et al. 2024 3.05 4.65 – 162 -0.630 – – –
Hunt & Reffert 2023 3.04 4.25 2.36 186 – – – –
Hao et al. 2022 – 3.96 – 251 0.498 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 436 100.0 251.04 -44.12 0.28 -2.49 -3.96 -53.4 0.56

💡 Note: The % column shows the percentage of members that OC 0668 shares with each listed object.

Visualization

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