MCM 77

(MCM2005b 77)

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0.11 UTI
0.0
CN
0.36
Cdens
0.25
CC3
0.0
Clit
0.92
Cdup
Stellar density (N50/rad) 1.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.36 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.92 Very likely unique

Overview

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MCM 77 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~2.74 kpc) differs significantly from the median photometric distance (~6.08 kpc).

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.92) 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 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster.

Mercer et al. (2005)
Association of stars. Detected using no magnitude cut. 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– 244.333 -50.53 0.364 -4.076 -4.087 -43.497
Morales et al. 2013 244.363 -50.511 – – – –
Mercer et al. 2005 244.367 -50.511 – – – –

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

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 6.08 – – – – – – –
Morales et al. 2013 6.08 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
DBSB 163 8.0 244.69 -50.31 0.34 -4.18 -4.16 – 0.1

💡 Note: The % column shows the percentage of members that MCM 77 shares with each listed object.

Visualization

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