ESO 493 03
(MWSC 1300)
0.21
UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
21
Core radius and density
2.3 [pc], 0.06 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.38 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
ESO 493 03 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.58 kpc) differs significantly from the median photometric distance (~1.40 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 | 114.916 | -27.325 | 0.152 | -1.456 | 2.143 | 89.856 |
| Just et al. | 2023 | 114.917 | -27.293 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -2.81 | 2.87 | â |
| Dib et al. | 2018 | 114.922 | -27.295 | â | â | â | â |
| Loktin & Popova | 2017 | 114.93 | -27.293 | â | -2.878 | 1.754 | 20.77 |
| Sampedro et al. | 2017 | 114.938 | -27.293 | â | â | â | â |
| Joshi et al. | 2016 | 114.922 | -27.295 | â | â | â | â |
| Kharchenko et al. | 2016 | 114.917 | -27.293 | â | â | â | â |
| Dias et al. | 2014 | 114.938 | -27.293 | â | -0.7 | 2.14 | 20.77 |
| Kharchenko et al. | 2013 | 114.922 | -27.295 | â | -0.6 | 1.64 | â |
| Piskunov et al. | 2008 | 114.919 | -27.287 | â | â | â | â |
| Kharchenko et al. | 2005 | 114.93 | -27.29 | â | 0.44 | 2.31 | â |
| Dias et al. | 2002 | 114.938 | -27.293 | â | -0.72 | 2.15 | 20.77 |
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 | 1.4 | 0.32 | â | 243 | â | 170 | â | â |
| Just et al. | 2023 | â | â | â | 243 | â | 101 | â | â |
| Dib et al. | 2018 | 1.40 | â | â | 243 | â | â | â | â |
| Loktin & Popova | 2017 | 2.29 | 1.25 | â | 209 | â | â | â | â |
| Joshi et al. | 2016 | 1.40 | 0.32 | â | 243 | â | 240 | â | â |
| Kharchenko et al. | 2016 | 1.40 | 0.32 | â | 243 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.40 | 0.32 | â | 243 | â | â | â | â |
| Piskunov et al. | 2008 | 1.40 | 0.32 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.40 | 0.32 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 1.40 | 0.32 | â | 398 | â | â | â | â |
MOCA
