ESO 165 09
(MWSC 1625)
0.25
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
7.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 165 09 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.54 kpc) differs significantly from the median photometric distance (~0.45 kpc).
Very close
Low extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 136.31 | -55.953 | 0.153 | -3.203 | 3.596 | â |
| Just et al. | 2023 | 136.346 | -55.935 | â | â | â | â |
| Bica et al. | 2019 | 136.31 | -55.952 | â | â | â | â |
| Loktin & Popova | 2017 | 136.305 | -55.955 | â | -10.15 | 10.47 | â |
| Kharchenko et al. | 2016 | 136.346 | -55.935 | â | â | â | â |
| Dias et al. | 2014 | 136.312 | -55.955 | â | -2.99 | 5.85 | â |
| Kharchenko et al. | 2013 | 136.35 | -55.938 | â | -9.83 | 10.62 | â |
| Piskunov et al. | 2008 | 136.297 | -55.958 | â | â | â | â |
| Kharchenko et al. | 2005 | 136.3 | -55.96 | â | -10.15 | 10.47 | â |
| Dias et al. | 2002 | 136.312 | -55.955 | â | -10.15 | 10.47 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 822 | â | 16 | â | â |
| Loktin & Popova | 2017 | 0.39 | 0.16 | â | 912 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.66 | 0.16 | â | 822 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.66 | 0.16 | â | 822 | â | â | â | â |
| Piskunov et al. | 2008 | 0.45 | 0.16 | â | 912 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.45 | 0.16 | â | 912 | â | â | â | â |
| Dias et al. | 2002 | 0.45 | 0.16 | â | 912 | â | â | â | â |
