OC 0095

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0.61 UTI
0.55
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 19.2 [N/pc2]
  • CN 0.55 Moderately 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 0095 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. 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– 304.145 29.779 0.543 -3.696 -5.625 43.96
Hunt & Reffert 2024 304.139 29.774 0.539 -3.705 -5.621 32.101
Cavallo et al. 2024 304.139 29.754 0.539 – – –
Hunt & Reffert 2023 304.139 29.774 0.539 -3.705 -5.621 32.101
Hao et al. 2022 304.141 29.739 0.542 -3.673 -5.583 –

💡 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– 1.945 4.32 2.65 32 0.432 700 – –
Hunt & Reffert 2024 – – – – – 700(1) – –
Cavallo et al. 2024 2.13 4.20 – 32 0.590 – – –
Hunt & Reffert 2023 1.76 4.33 2.65 55 – – – –
Hao et al. 2022 – 4.32 – 1 0.274 – – –

(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 500 100.0 304.15 29.78 0.54 -3.71 -5.63 43.96 0.08
CWWDL 4512 86.7 304.14 29.77 0.54 -3.71 -5.62 43.96 0.0

💡 Note: The % column shows the percentage of members that OC 0095 shares with each listed object.

Visualization

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