OCSN 92

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0.47 UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 5.5 [N/pc2]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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OCSN 92 is a moderately populated, very dense object of 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 near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 231.437 -36.115 7.147 -19.892 -23.809 1.775
Cavallo et al. 2024 231.102 -36.947 7.24 – – –
Hunt & Reffert 2023 231.555 -36.062 7.246 -20.498 -24.576 1.623
Qin et al. 2023 231.72 -35.96 7.26 -20.38 -23.75 1.05

💡 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– 0.14 0.26 0.58 16 -0.290 – – –
Cavallo et al. 2024 0.13 0.79 – 16 -0.290 – – –
Hunt & Reffert 2023 0.14 0.26 0.58 9 – – – –
Qin et al. 2023 0.14 0.06 – 20 – – – –

Visualization

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