OC 0629

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0.52 UTI
0.33
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0629 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity 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 – 230.116 -57.159 0.415 -4.177 -3.589 –
Hunt & Reffert 2024 230.108 -57.161 0.403 -4.171 -3.587 –
Cavallo et al. 2024 230.111 -57.16 0.402 – – –
Hunt & Reffert 2023 230.108 -57.161 0.403 -4.171 -3.587 –
Hao et al. 2022 230.119 -57.158 0.41 -4.179 -3.624 –

💡 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 – – – – – 941* – –
Cavallo et al. 2024 1.88 4.70 – 51 0.180 – – –
Hunt & Reffert 2023 2.33 4.89 2.10 23 – – – –
Hao et al. 2022 – 2.14 – 1 0.611 – – –

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

Visualization

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