AFGL5182

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0.20 UTI
0.44
CN
0.19
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.44 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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AFGL5182 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above 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 small percentage of members with at least one entry reported in the same catalogue. 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– 92.222 21.86 0.426 -0.176 -1.636 30.872
Bica et al. 2003 92.267 21.843 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
AFGL5180 18.2 92.18 21.68 0.36 -0.07 -1.48 30.87 0.11
CSS1a 11.4 92.28 21.84 0.4 0.06 -2.06 – 0.07

💡 Note: The % column shows the percentage of members that AFGL5182 shares with each listed object.

Visualization

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