OCSN 5

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0.08 UTI
0.6
CN
0.12
Cdens
0.75
CC3
0.0
Clit
0.27
Cdup
Core radius and density 2.4 [pc], 0.6 [pc-2]
  • CN 0.6 Moderately populated
  • Cdens 0.12 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.27 Possibly duplicate

Overview

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OCSN 5 is a moderately populated, very loose object of high 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant 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– 286.453 -16.597 4.083 0.851 -11.525 -24.126
Qin et al. 2023 286.21 -16.56 4.12 0.81 -11.69 -22.79

💡 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– 0.31 0.6 – 79 – – – –
Qin et al. 2023 0.31 0.60 – 79 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 222 73.2 286.45 -16.07 4.03 0.77 -11.1 -23.97 0.3

💡 Note: The % column shows the percentage of members that OCSN 5 shares with each listed object.

Visualization

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