ESO 175 06
(MWSC 2212)
0.34
UTI
0.0
CN
0.03
Cdens
0.38
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
6.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 175 06 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, above 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 (~5.78 kpc) differs significantly from the median photometric distance (~0.55 kpc).
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 | 214.598 | -56.927 | 0.173 | -5.686 | -2.273 | 35.324 |
| Just et al. | 2023 | 214.683 | -56.888 | â | â | â | â |
| Bica et al. | 2019 | 214.636 | -56.928 | â | â | â | â |
| Loktin & Popova | 2017 | 214.635 | -56.918 | â | -4.87 | -1.43 | -27.9 |
| Kharchenko et al. | 2016 | 214.683 | -56.888 | â | â | â | â |
| Dias et al. | 2014 | 214.633 | -56.918 | â | -4.87 | -1.43 | â |
| Kharchenko et al. | 2013 | 214.695 | -56.89 | â | -8.74 | -1.88 | -27.9 |
| Gozha et al. | 2012 | 214.633 | -56.918 | â | â | â | â |
| Piskunov et al. | 2008 | 214.671 | -56.922 | â | â | â | â |
| Kharchenko et al. | 2007 | 214.63 | -56.92 | â | 0.18 | â | -27.9 |
| Kharchenko et al. | 2005 | 214.68 | -56.92 | â | -8.65 | -2.43 | â |
| Dias et al. | 2002 | 214.633 | -56.918 | â | -4.87 | -1.43 | -27.9 |
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 | 398 | â | 12 | â | â |
| Loktin & Popova | 2017 | 0.41 | 0.62 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.59 | 0.58 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.59 | 0.58 | â | 398 | â | â | â | â |
| Gozha et al. | 2012 | 0.55 | â | â | 398 | â | 18 | â | â |
| Piskunov et al. | 2008 | 0.55 | 0.62 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.55 | 0.62 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 0.55 | 0.62 | â | 398 | â | â | â | â |
