AFGL5085

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0.21 UTI
0.29
CN
0.24
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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AFGL5085 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large 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 large 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– 42.537 62.064 0.167 -0.6 0.171 –
Bica et al. 2003 42.531 62.002 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0254 79.3 42.53 62.08 0.16 -0.6 0.16 – 0.03

💡 Note: The % column shows the percentage of members that AFGL5085 shares with each listed object.

Visualization

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