OCSN 23

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0.52 UTI
0.85
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.91
Cdup
Radius (P>50% members) 62.7 [arcmin]
  • CN 0.85 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.91 Very likely unique

Overview

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OCSN 23 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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 very likely a unique object, which shares a very small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Very close Low extinction Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 305.131 48.625 2.863 3.161 1.974 -7.704
Qin et al. 2023 305.3 48.52 2.89 3.3 2.02 -7.69

💡 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] Bfr BSS
Qin et al. 2023 0.39 0.34 – 32 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC-III 3723 52.6 304.16 46.65 2.92 3.51 1.72 -7.45 0.27
Theia 96 38.6 305.28 48.77 2.84 3.0 1.96 -7.96 0.0
RSG5 8.8 303.5 45.6 2.96 3.62 1.55 -7.39 0.89
OCSN 256 7.4 303.59 45.59 2.96 3.63 1.56 -7.39 0.01

💡 Note: The % column shows the percentage of members that OCSN 23 shares with each listed object.

Visualization

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