ESO 132 14
0.09
UTI
0.0
CN
0.34
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
1.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.34 Loose
- CC3 0.12 Very 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
ESO 132 14 is a sparse, loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 12 years.
(*): The parallax distance estimate (~2.65 kpc) differs significantly from the median photometric distance (~1.10 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 | 204.124 | -62.189 | 0.377 | -10.249 | -2.073 | -41.454 |
| Dias et al. | 2014 | 204.125 | -62.214 | â | -2.9 | -5.14 | â |
| Morales et al. | 2013 | 204.125 | -62.214 | â | â | â | â |
| Dias et al. | 2002 | 204.125 | -62.214 | â | -2.87 | -5.23 | 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 | 1.1 | 0.0 | â | 797 | â | â | â | â |
| Morales et al. | 2013 | 1.10 | â | â | 800 | â | â | â | â |
| Dias et al. | 2002 | 1.10 | 0.00 | â | 794 | â | â | â | â |
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.