OCSN 50

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0.41 UTI
0.33
CN
0.45
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 67.8 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OCSN 50 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Very close Low extinction Near-solar metallicity Young

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 – 62.11 21.466 5.156 5.663 -5.97 15.293
Zhang et al. 2024 62.36 21.42 – – – –
Cavallo et al. 2024 61.595 21.679 5.236 – – –
Hunt & Reffert 2023 62.36 21.42 5.24 5.817 -5.997 35.675
Qin et al. 2023 62.27 21.5 5.07 4.84 -6.04 14.52

💡 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
Zhang et al. 2024 – – – – 0.023* – – –
Cavallo et al. 2024 0.19 1.07 – 26 0.150 – – –
Hunt & Reffert 2023 0.20 0.75 0.71 20 – – – –
Qin et al. 2023 0.30 0.96 – 16 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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