VVVX CL090

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0.10 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

VVVX CL090 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below 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 8 years.

⚠️ 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.

No fundamental parameters

Borissova et al. (2018): Open cluster.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 274.313 -18.94 0.298 -1.282 -3.543 8.544
Borissova et al. 2018 274.313 -18.954

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

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.