Teutsch 55
(MWSC 200)
0.56
UTI
0.46
CN
1.0
Cdens
0.62
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
46
Core radius and density
0.7 [pc], 11 [pc-2]
- CN 0.46 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch 55 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 37.293 | 62.096 | 0.455 | -1.19 | -0.171 | -59.085 |
| Dias et al. | 2026 | 37.282 | 62.099 | 0.32 | -1.009 | -0.068 | -55.019 |
| Just et al. | 2023 | 37.338 | 62.068 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -1.11 | -0.29 | â |
| Loktin & Popova | 2017 | 37.245 | 62.094 | â | -0.961 | -2.646 | â |
| Sampedro et al. | 2017 | 37.25 | 62.094 | â | -0.85 | 0.83 | â |
| Kharchenko et al. | 2016 | 37.338 | 62.068 | â | â | â | â |
| Dias et al. | 2014 | 37.25 | 62.094 | â | -1.25 | 0.47 | â |
| Kharchenko et al. | 2013 | 37.35 | 62.07 | â | -0.2 | -2.63 | â |
| Kharchenko et al. | 2012 | 37.35 | 62.07 | â | -0.2 | -2.63 | â |
| Bukowiecki et al. | 2011 | 37.3 | 62.107 | â | â | â | â |
| Kronberger et al. | 2006 | 37.284 | 62.105 | â | â | â | â |
| Dias et al. | 2002 | 37.25 | 62.094 | â | -1.25 | 0.47 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.01 | 2.59 | â | 307 | -0.108 | 155 | â | â |
| Dias et al. | 2026 | 1.86 | 2.01 | â | 27 | -0.108 | â | â | â |
| Just et al. | 2023 | â | â | â | 543 | â | 151 | â | â |
| Loktin & Popova | 2017 | 1.18 | 1.48 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.01 | 2.82 | â | 543 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.01 | 2.82 | â | 543 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 159 | â | â |
| Kharchenko et al. | 2012 | 2.01 | 2.82 | â | 543 | â | â | â | â |
| Bukowiecki et al. | 2011 | 1.81(1) | 2.02 | â | 71 | â | â | â | â |
| Dias et al. | 2002 | 6.02 | 2.59 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.