MCM 32
(MCM2005b 32)
0.37
UTI
0.37
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
22.8 [N/pc2]
- CN 0.37 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate 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 32 is a poorly populated, very dense object of intermediate 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 significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 186.726 | -62.828 | 0.274 | -6.14 | -0.352 | -25.346 |
| Morales et al. | 2013 | 186.717 | -62.824 | â | â | â | â |
| Mercer et al. | 2005 | 186.72 | -62.824 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
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)
Associated with mid-IR extended emission. Cluster of stars. Detected using no magnitude cut. Appears in 2MASS images.