OC 0034

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0.55 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0034 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction 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 – 278.978 -12.8 0.517 0.37 -0.446 –
Hunt & Reffert 2024 278.985 -12.8 0.517 0.377 -0.451 -18.732
Cavallo et al. 2024 278.977 -12.801 0.518 – – –
Hunt & Reffert 2023 278.985 -12.8 0.517 0.377 -0.451 -18.732
Hao et al. 2022 278.995 -12.8 0.529 0.333 -0.513 3.648

💡 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 – – – – – 298* – –
Cavallo et al. 2024 1.79 1.39 – 151 0.510 – – –
Hunt & Reffert 2023 1.84 1.94 0.93 75 – – – –
Hao et al. 2022 – 2.38 – 40 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 13352 72.0 278.97 -12.8 0.52 0.33 -0.48 -18.73 0.11

💡 Note: The % column shows the percentage of members that OC 0034 shares with each listed object.

Visualization

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