Auner 1
(MWSC 1087; ESO 558 08)
0.88
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
0.9 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Auner 1 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-poor, old cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~10.93 kpc) differs significantly from the median photometric distance (~8.18 kpc).
Very distant
Moderate extinction
Massive
Metal-poor
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 106.061 | -19.749 | 0.091 | -0.312 | 0.989 | 134.816 |
| Hu & Soubiran | 2025 | 106.057 | -19.759 | â | â | â | â |
| Hunt & Reffert | 2024 | 106.064 | -19.747 | 0.1 | -0.304 | 0.99 | 133.439 |
| Cavallo et al. | 2024 | 106.057 | -19.759 | 0.097 | â | â | â |
| Hunt & Reffert | 2023 | 106.064 | -19.747 | 0.1 | -0.304 | 0.99 | 133.439 |
| Just et al. | 2023 | 106.054 | -19.742 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 106.06 | -19.748 | 0.093 | -0.28 | 1.015 | â |
| Cantat-Gaudin & Anders | 2020 | 106.06 | -19.748 | 0.093 | -0.28 | 1.015 | â |
| Bica et al. | 2019 | 106.068 | -19.742 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 106.06 | -19.748 | 0.093 | -0.28 | 1.015 | â |
| Loktin & Popova | 2017 | 106.08 | -19.75 | â | 3.706 | 3.77 | â |
| Kharchenko et al. | 2016 | 106.054 | -19.742 | â | â | â | â |
| Dias et al. | 2014 | 106.067 | -19.75 | â | -1.85 | 0.45 | â |
| Kharchenko et al. | 2013 | 106.06 | -19.744 | â | 0.97 | 4.01 | â |
| Gozha et al. | 2012 | 106.067 | -19.75 | â | â | â | â |
| Dias et al. | 2002 | 106.067 | -19.75 | â | -1.85 | 0.45 | 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 | -0.380* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 873* | â | â |
| Cavallo et al. | 2024 | 8.36 | 1.00 | â | 2455 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 7.82 | 1.61 | 1.95 | 1233 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2239 | â | 5117 | â | â |
| Cantat-Gaudin et al. | 2020 | 8.99 | 0.99 | â | 3090 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.18 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.18 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.40 | 1.71 | â | 525 | â | â | â | â |
| Kharchenko et al. | 2016 | 7.15 | 1.23 | â | 2239 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.15 | 1.23 | â | 2239 | -0.500 | â | â | â |
| Gozha et al. | 2012 | 8.90 | â | â | 3236 | -0.500 | â | â | â |
| Dias et al. | 2002 | 8.90 | 0.99 | â | 3236 | -0.500 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.