Teutsch 5
(MWSC 438; DSH J0455.7+3646; FSR 0747)
0.77
UTI
0.76
CN
1.0
Cdens
0.5
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.9 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Teutsch 5 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 73.941 | 36.784 | 0.456 | 0.07 | -1.575 | -72.2 |
| Hu & Soubiran | 2025 | 73.943 | 36.773 | â | â | â | â |
| Hunt & Reffert | 2024 | 73.941 | 36.783 | 0.445 | 0.091 | -1.574 | -72.128 |
| Cavallo et al. | 2024 | 73.943 | 36.773 | 0.443 | â | â | â |
| Hunt & Reffert | 2023 | 73.941 | 36.783 | 0.445 | 0.091 | -1.574 | -72.128 |
| Just et al. | 2023 | 73.923 | 36.783 | â | â | â | â |
| Donor et al. | 2020 | 73.932 | 36.783 | â | 0.23 | -1.46 | -74.7 |
| Bica et al. | 2019 | 73.924 | 36.782 | â | â | â | â |
| Loktin & Popova | 2017 | 73.935 | 36.782 | â | -0.205 | -6.685 | â |
| Kharchenko et al. | 2016 | 73.923 | 36.783 | â | â | â | â |
| Dias et al. | 2014 | 73.929 | 36.782 | â | -0.94 | -1.72 | â |
| Kharchenko et al. | 2013 | 73.932 | 36.783 | â | -0.79 | -6.23 | â |
| Kharchenko et al. | 2012 | 73.932 | 36.783 | â | -0.77 | -6.4 | â |
| Kronberger et al. | 2006 | 73.93 | 36.782 | â | â | â | â |
| Dias et al. | 2002 | 73.929 | 36.782 | â | -0.9 | -1.72 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | 0.030* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 544* | â | â |
| Cavallo et al. | 2024 | 2.44 | 2.57 | â | 1380 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 2.01 | 2.59 | 2.39 | 1007 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2399 | â | 641 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.350 | â | â | â |
| Loktin & Popova | 2017 | 1.54 | 2.67 | â | 1096 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.00 | 1.86 | â | 2399 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.00 | 1.86 | â | 2399 | â | â | â | â |
| Kharchenko et al. | 2012 | 3.00 | 1.86 | â | 2399 | â | â | â | â |
| Dias et al. | 2002 | 2.33 | 2.39 | â | 2239 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.