OCSN 26

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0.02 UTI
0.26
CN
0.45
Cdens
0.5
CC3
0.0
Clit
0.08
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

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OCSN 26 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large 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– 338.708 29.946 3.123 -7.909 -4.35 4.995
Qin et al. 2023 338.68 29.92 3.13 -8.08 -4.44 6.06

💡 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– 0.33 0.28 – 891 – – – –
Qin et al. 2023 0.33 0.28 – 891 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1188 92.3 338.71 29.92 3.11 -7.87 -4.35 4.99 0.38

💡 Note: The % column shows the percentage of members that OCSN 26 shares with each listed object.

Visualization

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