OC 0064

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0.20 UTI
0.54
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.36
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.36 Possibly duplicate

Overview

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OC 0064 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Very high 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 – 282.461 -0.333 0.49 -0.398 -1.965 -31.625
Hunt & Reffert 2024 282.466 -0.331 0.461 -0.385 -1.899 -35.34
Cavallo et al. 2024 282.476 -0.335 0.458 – – –
Hunt & Reffert 2023 282.466 -0.331 0.461 -0.385 -1.899 -35.34
Hao et al. 2022 282.464 -0.328 0.54 -0.397 -1.938 –

💡 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 – – – – – 1536* – –
Cavallo et al. 2024 2.06 5.06 – 39 0.480 – – –
Hunt & Reffert 2023 2.05 5.17 2.85 35 – – – –
Hao et al. 2022 – 4.32 – 1 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2352 87.9 282.46 -0.33 0.48 -0.42 -1.98 -31.63 0.07
FoF 2172 63.8 282.46 -0.32 0.48 -0.4 -1.92 -163.47 0.43

💡 Note: The % column shows the percentage of members that OC 0064 shares with each listed object.

Visualization

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