MCM 3
0.08
UTI
0.0
CN
0.16
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
17
Core radius and density
2.5 [pc], 0.8 [pc-2]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- 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 3 is a sparse, very loose object of 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 21 years.
Note: This object shares a small percentage of members with 3 later reported entries. See table with shared members information.
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 | 274.707 | -17.049 | 0.608 | -0.615 | -2.171 | 15.3 |
| Mercer et al. | 2005 | 274.627 | -16.976 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
Mercer et al. (2005)
Cluster of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm.