OC 0107

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0.31 UTI
0.3
CN
0.38
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0107 is a poorly populated, loose object of low 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 age 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– 305.032 36.187 0.551 -2.369 -4.482 –
Hunt & Reffert 2024 305.037 36.21 0.552 -2.362 -4.476 –
Cavallo et al. 2024 305.015 36.166 0.551 – – –
Hunt & Reffert 2023 305.037 36.21 0.552 -2.362 -4.476 –
Hao et al. 2022 305.059 36.21 0.554 -2.397 -4.529 –

💡 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– 1.645 2.69 0.84 48 0.363 191 – –
Hunt & Reffert 2024 – – – – – 191(1) – –
Cavallo et al. 2024 1.52 2.84 – 49 0.270 – – –
Hunt & Reffert 2023 1.77 2.69 0.84 48 – – – –
Hao et al. 2022 – 1.70 – 2 0.457 – – –

(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 271 83.3 305.05 36.15 0.55 -2.33 -4.46 – 0.07

💡 Note: The % column shows the percentage of members that OC 0107 shares with each listed object.

Visualization

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