ESO 494 09
(MWSC 1400)
0.64
UTI
0.29
CN
1.0
Cdens
0.62
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.29 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 494 09 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~2.06 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate 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 | 119.738 | -27.661 | 0.337 | -2.562 | 3.79 | 36.926 |
| Hu & Soubiran | 2025 | 119.71 | -27.645 | â | â | â | â |
| Hunt & Reffert | 2024 | 119.726 | -27.673 | 0.341 | -2.563 | 3.806 | 36.864 |
| Cavallo et al. | 2024 | 119.71 | -27.645 | 0.34 | â | â | â |
| Hunt & Reffert | 2023 | 119.726 | -27.673 | 0.341 | -2.563 | 3.806 | 36.864 |
| Just et al. | 2023 | 119.811 | -27.581 | â | â | â | â |
| Bica et al. | 2019 | 119.811 | -27.584 | â | â | â | â |
| Loktin & Popova | 2017 | 119.82 | -27.582 | â | -1.557 | 2.311 | â |
| Kharchenko et al. | 2016 | 119.811 | -27.581 | â | â | â | â |
| Dias et al. | 2014 | 119.817 | -27.585 | â | -1.77 | 3.51 | â |
| Kharchenko et al. | 2013 | 119.817 | -27.583 | â | -2.62 | 1.0 | â |
| Dias et al. | 2002 | 119.817 | -27.585 | â | -1.78 | 3.5 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.120* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 337* | â | â |
| Cavallo et al. | 2024 | 2.83 | 1.51 | â | 589 | 0.430 | â | â | â |
| Hunt & Reffert | 2023 | 2.78 | 1.39 | 1.20 | 619 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 543 | â | 107 | â | â |
| Loktin & Popova | 2017 | 2.21 | 0.70 | â | 977 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.91 | 0.97 | â | 543 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.91 | 0.97 | â | 543 | â | â | â | â |
| Dias et al. | 2002 | 1.21 | 1.30 | â | 63 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.