VVVX CL095

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0.05 UTI
0.0
CN
0.14
Cdens
0.12
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

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VVVX CL095 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close 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 8 years.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a very small percentage 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=0.88) 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)
Small group around YSO: SSTGLMA G014.0632-00.5199.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 274.402 -16.931 0.523 -0.271 -2.162 -11.404
Borissova et al. 2018 274.481 -16.976 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ryu 210 16.0 274.31 -16.91 0.56 -0.78 -2.23 13.88 0.14
MCM 3 12.0 274.71 -17.05 0.61 -0.61 -2.17 15.3 0.25
VVVX CL097 4.0 274.52 -16.84 0.62 0.14 -1.82 0.43 0.33

💡 Note: The % column shows the percentage of members that VVVX CL095 shares with each listed object.

Visualization

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