OCSN 45

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0.06 UTI
0.0
CN
0.13
Cdens
0.38
CC3
0.0
Clit
0.6
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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OCSN 45 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 21.03 62.016 2.61 7.833 -4.104 -3.017
Qin et al. 2023 22.15 61.9 2.64 7.79 -4.1 -3.38

💡 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– 0.52 0.71 – 45 – – – –
Qin et al. 2023 0.52 0.71 – 45 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 446 40.0 18.39 62.72 2.57 7.78 -3.73 -3.67 0.33

💡 Note: The % column shows the percentage of members that OCSN 45 shares with each listed object.

Visualization

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