MCM 14
(MCM2005b 14)
0.21
UTI
0.26
CN
0.52
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
26
Core radius and density
1.2 [pc], 2.6 [pc-2]
- CN 0.26 Poorly populated
- Cdens 0.52 Moderately dense
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
MCM 14 is a poorly populated, moderately dense 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.
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 | 284.527 | 1.61 | 0.479 | -0.386 | -2.376 | -85.696 |
| Morales et al. | 2013 | 284.526 | 1.613 | â | â | â | â |
| Mercer et al. | 2005 | 284.525 | 1.611 | 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 | 2.21 | â | â | â | â | â | â | â |
| Morales et al. | 2013 | 2.21 | â | â | â | â | â | â | â |
Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.
Mercer et al. (2005)
Associated with mid-IR extended emission. Cluster of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm. Detected using 'bright' 3.6m magnitude cut.