BFS56

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0.24 UTI
0.46
CN
0.47
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.4 [N/pc2]
  • CN 0.46 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
BFS56 is a poorly populated, loose 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 23 years.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.914 -3.946 0.389 -0.647 -1.183 42.999
Bica et al. 2003 104.801 -3.914 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1512 50.0 105.01 -3.97 0.38 -0.64 -1.18 42.1 0.08

💡 Note: The % column shows the percentage of members that BFS56 shares with each listed object.

Visualization

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