OCSN 98

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0.55 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 22.9 [N/pc2]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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OCSN 98 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 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.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Cavallo et al. (2024)
Silver 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– 241.26 -19.698 6.561 -9.892 -21.689 -7.92
Cavallo et al. 2024 241.261 -19.717 6.564 – – –
Hunt & Reffert 2023 241.301 -19.743 6.564 -9.986 -21.698 -10.865
Qin et al. 2023 241.3 -19.78 6.6 -9.86 -21.76 -6.78

💡 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– 0.15 0.56 0.74 7 -0.370 – – –
Cavallo et al. 2024 0.15 1.49 – 8 -0.370 – – –
Hunt & Reffert 2023 0.15 0.56 0.74 4 – – – –
Qin et al. 2023 0.17 0.31 – 7 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 96 1.7 240.86 -22.58 7.02 -11.74 -23.9 -7.43 0.67

💡 Note: The % column shows the percentage of members that OCSN 98 shares with each listed object.

Visualization

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