MCM 68
(fsr 1712; MCM2005b 68; MWSC 2332; GLIMPSE 68; Mercer 68)
0.15
UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.23
Clit
1.0
Cdup
Stellar density (N50/rad)
0.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.15 Very loose
- CC3 0.12 Very low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
MCM 68 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~2.69 kpc) differs significantly from the median photometric distance (~1.14 kpc).
â 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 238.658 | -52.544 | 0.371 | -5.734 | -5.228 | â |
| Just et al. | 2023 | 238.668 | -52.479 | â | â | â | â |
| Bica et al. | 2019 | 238.694 | -52.528 | â | â | â | â |
| Dib et al. | 2018 | 238.68 | -52.48 | â | â | â | â |
| Joshi et al. | 2016 | 238.68 | -52.48 | â | â | â | â |
| Kharchenko et al. | 2016 | 238.668 | -52.479 | â | â | â | â |
| Kharchenko et al. | 2013 | 238.68 | -52.48 | â | -4.57 | -2.67 | â |
| Morales et al. | 2013 | 238.692 | -52.53 | â | â | â | â |
| Froebrich et al. | 2007 | 238.692 | -52.502 | â | â | â | â |
| Mercer et al. | 2005 | 238.695 | -52.53 | â | â | â | â |
đĄ 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 | 99999â | 1.14 | 2.17 | â | 398 | â | 76 | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 76 | â | â |
| Dib et al. | 2018 | 1.14 | â | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 1.14 | 2.17 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.14 | 2.17 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.14 | 2.17 | â | 398 | â | â | â | â |
| Morales et al. | 2013 | 1.80 | â | â | 1000 | â | â | â | â |
MOCA

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)
Cluster of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm.