ESO 313 03
(MWSC 1499)
0.25
UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
5.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.12 Very low quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 313 03 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.72 kpc) differs significantly from the median photometric distance (~4.27 kpc).
Distant
High extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 127.915 | -41.784 | 0.149 | -3.174 | 3.504 | 94.606 |
| Just et al. | 2023 | 127.903 | -41.784 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 127.907 | -41.784 | 0.163 | -3.189 | 3.492 | â |
| Cantat-Gaudin & Anders | 2020 | 127.907 | -41.784 | 0.163 | -3.189 | 3.492 | â |
| Bica et al. | 2019 | 127.925 | -41.784 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 127.907 | -41.784 | 0.163 | -3.189 | 3.492 | â |
| Kharchenko et al. | 2016 | 127.903 | -41.784 | â | â | â | â |
| Dias et al. | 2014 | 127.921 | -41.792 | â | -1.01 | 0.01 | â |
| Kharchenko et al. | 2013 | 127.908 | -41.787 | â | -2.22 | 4.67 | â |
| Dias et al. | 2002 | 127.921 | -41.792 | â | -2.22 | 4.67 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 398 | â | 339 | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.20 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.20 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.27 | 3.36 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.27 | 3.36 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 3.05 | 2.85 | â | 708 | â | â | â | â |

