ESO 311 14
(MWSC 1352)
0.19
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
13
Core radius and density
6.0 [pc], 0.03 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
ESO 311 14 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.44 kpc) differs significantly from the median photometric distance (~1.28 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 | 117.36 | -42.679 | 0.155 | -2.096 | 2.843 | 59.196 |
| Just et al. | 2023 | 117.345 | -42.682 | â | â | â | â |
| Bica et al. | 2019 | 117.348 | -42.697 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -3.99 | 4.25 | â |
| Dib et al. | 2018 | 117.349 | -42.685 | â | â | â | â |
| Loktin & Popova | 2017 | 117.345 | -42.685 | â | -3.012 | 5.429 | â |
| Sampedro et al. | 2017 | 117.35 | -42.705 | â | -5.06 | 2.85 | â |
| Joshi et al. | 2016 | 117.349 | -42.685 | â | â | â | â |
| Kharchenko et al. | 2016 | 117.345 | -42.682 | â | â | â | â |
| Dias et al. | 2014 | 117.35 | -42.705 | â | -5.12 | 2.33 | â |
| Kharchenko et al. | 2013 | 117.349 | -42.685 | â | -1.12 | 5.58 | â |
| Bukowiecki et al. | 2011 | 117.325 | -42.697 | â | â | â | â |
| Dias et al. | 2002 | 117.35 | -42.705 | â | -5.86 | 3.15 | 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 | 1.28 | 0.66 | â | 55 | â | 111 | â | â |
| Just et al. | 2023 | â | â | â | 55 | â | 31 | â | â |
| Dib et al. | 2018 | 1.28 | â | â | 55 | â | â | â | â |
| Loktin & Popova | 2017 | 3.62 | 0.86 | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 1.28 | 0.66 | â | 55 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.28 | 0.66 | â | 55 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.28 | 0.66 | â | 55 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 191 | â | â |
| Bukowiecki et al. | 2011 | 1.61(1) | 0.28 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 1.61 | 0.32 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
