OCSN 284

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0.00 UTI
0.65
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 19.6 [N/pc2]
  • CN 0.65 Moderately 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 284 is a moderately populated, very dense object of very 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 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– 56.448 29.825 2.49 2.68 -5.242 18.547
Qin et al. 2023 56.33 29.74 2.48 2.62 -5.28 17.47

💡 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– 0.57 0.87 – 5 – – – –
Qin et al. 2023 0.57 0.87 – 5 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi Teutsch 10 100.0 56.43 29.82 2.49 2.69 -5.24 18.55 0.7
UBC 19 93.8 56.44 29.82 2.47 2.66 -5.23 17.24 0.0
OC 0278 56.2 56.37 29.78 2.47 2.57 -5.26 18.05 0.0

💡 Note: The % column shows the percentage of members that OCSN 284 shares with each listed object.

Visualization

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