ESO 430 18
(MWSC 1431)
0.45
UTI
0.25
CN
0.22
Cdens
0.5
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.22 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 430 18 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.14 kpc) differs significantly from the median photometric distance (~0.87 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 121.791 | -30.878 | 0.241 | -2.595 | 3.231 | 50.361 |
| Hunt & Reffert | 2024 | 121.726 | -30.876 | 0.227 | -2.599 | 3.25 | â |
| Cavallo et al. | 2024 | 121.799 | -30.874 | 0.233 | â | â | â |
| Hunt & Reffert | 2023 | 121.726 | -30.876 | 0.227 | -2.599 | 3.25 | â |
| Just et al. | 2023 | 121.757 | -30.832 | â | â | â | â |
| Bica et al. | 2019 | 121.718 | -30.837 | â | â | â | â |
| Kharchenko et al. | 2016 | 121.757 | -30.832 | â | â | â | â |
| Dias et al. | 2014 | 121.717 | -30.837 | â | -2.56 | 0.86 | â |
| Kharchenko et al. | 2013 | 121.762 | -30.835 | â | -6.25 | -0.54 | â |
| Piskunov et al. | 2008 | 121.701 | -30.834 | â | â | â | â |
| Piskunov et al. | 2007 | 121.701 | -30.834 | â | â | â | â |
| Kharchenko et al. | 2005 | 121.71 | -30.84 | â | -7.91 | -0.81 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 132* | â | â |
| Cavallo et al. | 2024 | 3.39 | 1.09 | â | 100 | -0.330 | â | â | â |
| Hunt & Reffert | 2023 | 4.13 | 0.66 | 2.08 | 85 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 750 | â | 81 | â | â |
| Kharchenko et al. | 2016 | 0.87 | 0.00 | â | 750 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.87 | 0.00 | â | 750 | â | â | â | â |
| Piskunov et al. | 2008 | 0.83 | 0.00 | â | 1122 | â | 23* | â | â |
| Piskunov et al. | 2007 | 0.83 | 0.00 | â | 1122 | â | 5 | â | â |
| Kharchenko et al. | 2005 | 0.83 | 0.00 | â | 1122 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.