OC 0639

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0.00 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 6.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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OC 0639 is a sparse, very dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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, and a moderate percentage with at least one entry reported in the same catalogue. 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– 261.066 -62.461 2.042 -0.423 -8.969 8.852
Hao et al. 2022 261.147 -62.418 2.04 -0.419 -8.992 12.187

💡 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– – 1.54 – 63 0.274 – – –
Hao et al. 2022 – 1.54 – 63 0.274 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi 24 100.0 260.78 -62.72 2.06 -0.45 -8.98 9.22 0.97
OC 0638 32.0 261.0 -62.86 2.07 -0.34 -8.94 6.93 0.0
LISC-III 3249 8.0 260.88 -62.08 2.06 -0.56 -8.74 9.26 0.05

💡 Note: The % column shows the percentage of members that OC 0639 shares with each listed object.

Visualization

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