ESO 260 17
(MWSC 1624)
0.21
UTI
0.28
CN
0.07
Cdens
0.12
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
28
Core radius and density
1.4 [pc], 0.3 [pc-2]
- CN 0.28 Poorly populated
- Cdens 0.07 Very loose
- CC3 0.12 Very low quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
ESO 260 17 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~1.81 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 | 136.241 | -46.049 | 0.337 | -3.385 | 3.503 | 11.306 |
| Just et al. | 2023 | 136.183 | -46.032 | â | â | â | â |
| Bica et al. | 2019 | 136.206 | -46.043 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -6.42 | 4.04 | â |
| Dib et al. | 2018 | 136.188 | -46.035 | â | â | â | â |
| Sampedro et al. | 2017 | 136.204 | -46.042 | â | -0.03 | 3.49 | â |
| Kharchenko et al. | 2016 | 136.183 | -46.032 | â | â | â | â |
| Dias et al. | 2014 | 136.204 | -46.042 | â | 0.15 | 4.14 | â |
| Kharchenko et al. | 2013 | 136.188 | -46.035 | â | -5.68 | 6.0 | â |
| Bukowiecki et al. | 2011 | 136.213 | -46.102 | â | â | â | â |
| Dias et al. | 2002 | 136.204 | -46.042 | â | 0.15 | 4.14 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.81 | 2.44 | â | 977 | â | 356 | â | â |
| Just et al. | 2023 | â | â | â | 977 | â | 56 | â | â |
| Dib et al. | 2018 | 1.81 | â | â | 977 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.81 | 2.10 | â | 977 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.81 | 2.10 | â | 977 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 657 | â | â |
| Bukowiecki et al. | 2011 | 1.38(1) | 2.78 | â | 71 | â | â | â | â |
| Dias et al. | 2002 | 1.37 | 2.84 | â | 71 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
