OC 0019

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0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.1 [N/pc2]
  • CN 0.0 Sparse
  • 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 0019 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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

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 99999– 274.104 -20.149 0.52 1.15 -0.367 –
Hunt & Reffert 2024 274.107 -20.144 0.522 1.134 -0.396 –
Cavallo et al. 2024 274.12 -20.133 0.526 – – –
Hunt & Reffert 2023 274.107 -20.144 0.522 1.134 -0.396 –
Hao et al. 2022 274.116 -20.138 0.521 1.169 -0.313 –

💡 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] Bfrac BSS
UCC 99999– 1.615 2.74 2.25 62 0.175 322 – –
Hunt & Reffert 2024 – – – – – 322(1) – –
Cavallo et al. 2024 1.43 2.82 – 62 -0.260 – – –
Hunt & Reffert 2023 1.80 2.20 2.25 87 – – – –
Hao et al. 2022 – 2.74 – 32 0.611 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 191 100.0 274.1 -20.18 0.51 1.13 -0.38 -15.74 0.43

💡 Note: The % column shows the percentage of members that OC 0019 shares with each listed object.

Visualization

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