Teutsch 28
(MWSC 3347; DSH J2028.2+3506)
0.81
UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.2 [arcmin]
- CN 0.72 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Teutsch 28 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Distant
Very high extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 307.065 | 35.111 | 0.245 | -2.248 | -4.082 | -28.995 |
| Hunt & Reffert | 2024 | 307.067 | 35.113 | 0.261 | -2.339 | -4.148 | -29.479 |
| Cavallo et al. | 2024 | 307.05 | 35.118 | 0.267 | â | â | â |
| Hunt & Reffert | 2023 | 307.067 | 35.113 | 0.261 | -2.339 | -4.148 | -29.479 |
| Just et al. | 2023 | 307.064 | 35.11 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 307.059 | 35.103 | 0.242 | -2.076 | -3.936 | â |
| Cantat-Gaudin & Anders | 2020 | 307.059 | 35.103 | 0.242 | -2.076 | -3.936 | â |
| Soubiran et al. | 2018 | 307.059 | 35.103 | â | â | â | -18.55 |
| Bica et al. | 2019 | 307.072 | 35.114 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 307.059 | 35.103 | 0.242 | -2.076 | -3.936 | â |
| Loktin & Popova | 2017 | 307.08 | 35.115 | â | -0.405 | -1.129 | â |
| Kharchenko et al. | 2016 | 307.064 | 35.11 | â | â | â | â |
| Kharchenko et al. | 2013 | 307.069 | 35.112 | â | -1.3 | -3.48 | â |
| Kronberger et al. | 2006 | 307.069 | 35.114 | â | â | â | â |
| Dias et al. | 2002 | 307.079 | 35.115 | â | 3.02 | -0.83 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1201* | â | â |
| Cavallo et al. | 2024 | 3.53 | 5.28 | â | 257 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 3.24 | 5.46 | 2.33 | 210 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 708 | â | 1429 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.17 | 3.74 | â | 1905 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.69 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.69 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.69 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.16 | 3.22 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.80 | 5.81 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.80 | 5.81 | â | 708 | â | â | â | â |
| Dias et al. | 2002 | 3.10 | 4.46 | â | 8913 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.