OCSN 193

(epsCha)

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0.00 UTI
0.31
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 29.7 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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OCSN 193 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a very young cluster (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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 180.229 -78.342 9.769 -41.233 -6.05 13.812
Qin et al. 2023 180.34 -78.47 9.78 -40.74 -6.64 -15.0

💡 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– 0.12 0.31 – 8 – – – –
Qin et al. 2023 0.12 0.31 – 8 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Feigelson 1 100.0 180.43 -76.37 9.74 -40.27 -6.17 13.74 0.69
HSC 2515 74.2 180.23 -78.74 9.81 -41.36 -5.78 15.01 0.0

💡 Note: The % column shows the percentage of members that OCSN 193 shares with each listed object.

Visualization

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