OCSN 31

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0.00 UTI
0.26
CN
0.49
Cdens
0.62
CC3
0.25
Clit
0.0
Cdup
Stellar density (N50/rad) 2.4 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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OCSN 31 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (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.

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– 330.055 50.774 3.637 9.54 -0.475 -5.466
Zhang et al. 2024 329.656 50.786 – – – –
Cavallo et al. 2024 330.917 51.335 3.676 – – –
Hunt & Reffert 2023 329.656 50.786 3.649 9.603 -0.444 -8.846
Qin et al. 2023 329.53 50.84 3.58 9.68 -0.36 -5.2

💡 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– 0.28 0.28 0.41 37 -0.169 – – –
Zhang et al. 2024 – – – – -0.428(1) – – –
Cavallo et al. 2024 0.28 0.43 – 37 0.090 – – –
Hunt & Reffert 2023 0.26 0.11 0.41 74 – – – –
Qin et al. 2023 0.30 0.28 – 32 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 136 100.0 330.17 51.09 3.64 9.54 -0.41 -4.86 0.31

💡 Note: The % column shows the percentage of members that OCSN 31 shares with each listed object.

Visualization

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