OCSN 77

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0.07 UTI
0.47
CN
0.67
Cdens
1.0
CC3
0.25
Clit
0.13
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.47 Poorly populated
  • Cdens 0.67 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.13 Likely duplicate

Overview

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OCSN 77 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously 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– 112.552 -12.517 1.873 -5.823 -1.004 17.558
Hunt & Reffert 2024 112.661 -12.54 1.825 -5.767 -1.022 15.407
Cavallo et al. 2024 112.463 -12.497 1.843 – – –
Hunt & Reffert 2023 112.661 -12.54 1.825 -5.767 -1.022 15.407
Qin et al. 2023 112.66 -12.82 1.88 -5.79 -0.99 15.22

💡 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– 0.55 0.4 0.79 126 0.230 197 – –
Hunt & Reffert 2024 – – – – – 197(1) – –
Cavallo et al. 2024 0.55 0.45 – 126 0.230 – – –
Hunt & Reffert 2023 0.52 0.13 0.79 132 – – – –
Qin et al. 2023 0.62 0.40 – 100 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2424 87.2 112.51 -12.56 1.88 -5.81 -0.99 17.56 0.36
CWWDL 14639 76.6 112.41 -12.37 1.88 -5.83 -1.02 16.02 0.08

💡 Note: The % column shows the percentage of members that OCSN 77 shares with each listed object.

Visualization

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