Ryu 834

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0.21 UTI
0.0
CN
0.86
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Stellar density (N50/rad) 4.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.86 Dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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Ryu 834 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 278.512 -8.186 0.311 -1.104 -3.183 34.104
Bica et al. 2019 278.544 -8.181 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 119 4.0 278.44 -8.13 0.32 -0.96 -3.42 5.56 0.08

💡 Note: The % column shows the percentage of members that Ryu 834 shares with each listed object.

Visualization

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