Teutsch 162
(MWSC 232)
0.27
UTI
0.3
CN
0.04
Cdens
0.12
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.3 Poorly populated
- Cdens 0.04 Very loose
- CC3 0.12 Very low quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch 162 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.39 kpc) differs significantly from the median photometric distance (~1.60 kpc).
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 41.876 | 62.023 | 0.185 | -0.893 | 0.431 | -71.573 |
| Just et al. | 2023 | 41.904 | 61.971 | â | â | â | â |
| Loktin & Popova | 2017 | 41.91 | 61.975 | â | -0.716 | -1.357 | â |
| Kharchenko et al. | 2016 | 41.904 | 61.971 | â | â | â | â |
| Dias et al. | 2014 | 41.917 | 61.975 | â | -0.65 | -1.98 | â |
| Kharchenko et al. | 2013 | 41.917 | 61.973 | â | -1.45 | -1.56 | â |
| Kharchenko et al. | 2012 | 41.917 | 61.973 | â | -1.45 | -1.56 | â |
| Kronberger et al. | 2006 | 41.926 | 61.975 | â | â | â | â |
| Dias et al. | 2002 | 41.917 | 61.975 | â | -0.65 | -1.98 | 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 | 1.6 | 2.94 | â | 10 | â | 13 | â | â |
| Just et al. | 2023 | â | â | â | 10 | â | 13 | â | â |
| Loktin & Popova | 2017 | 1.66 | 1.25 | â | 16 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.60 | 2.94 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.60 | 2.94 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.60 | 2.94 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 2.05 | 1.58 | â | 10 | â | â | â | â |
MOCA
