MCM 86

(MCM2005b 86)

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0.04 UTI
0.0
CN
0.08
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
MCM 86 is a sparse, very loose object of very 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 13 years.

Note: This object shares a very small 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.

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Mercer et al. (2005)
Association of stars. Detected in 2MASS catalog with our algorithm.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 256.144 -41.704 0.403 -1.962 -3.313 -9.686
Morales et al. 2013 256.167 -41.706 – – – –
Mercer et al. 2005 256.169 -41.706 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
G3CC 40 4.0 256.31 -41.48 0.4 -1.62 -3.45 0.51 0.04

💡 Note: The % column shows the percentage of members that MCM 86 shares with each listed object.

Visualization

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