Teutsch 52
(MWSC 561; DSH J0530.3+3813)
0.57
UTI
0.31
CN
1.0
Cdens
0.12
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
1.1 [arcmin]
- CN 0.31 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.12 Very low quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 52 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.68 kpc) differs significantly from the median photometric distance (~4.20 kpc).
Distant
High extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 82.575 | 38.228 | 0.15 | -0.022 | -0.351 | β |
| Just et al. | 2023 | 82.549 | 38.208 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 82.575 | 38.244 | 0.158 | 0.059 | -0.136 | β |
| SΓ‘nchez et al. | 2020 | 82.575 | 38.231 | β | 0.266 | -0.41 | β |
| Cantat-Gaudin & Anders | 2020 | 82.575 | 38.244 | 0.158 | 0.059 | -0.136 | β |
| Bica et al. | 2019 | 82.572 | 38.231 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 82.575 | 38.244 | 0.158 | 0.059 | -0.136 | β |
| Kharchenko et al. | 2016 | 82.549 | 38.208 | β | β | β | β |
| Dias et al. | 2014 | 82.575 | 38.231 | β | -0.89 | -2.25 | β |
| Kharchenko et al. | 2013 | 82.56 | 38.207 | β | -1.85 | -2.71 | β |
| Kharchenko et al. | 2012 | 82.56 | 38.207 | β | -1.85 | -2.71 | β |
| Kronberger et al. | 2006 | 82.576 | 38.231 | β | β | β | β |
| Dias et al. | 2002 | 82.575 | 38.231 | β | -0.9 | -2.27 | β |
π‘ 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 | β | β | β | 631 | β | 164 | β | β |
| Cantat-Gaudin & Anders | 2020 | 5.34 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 5.34 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 4.20 | 3.35 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.20 | 3.35 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2012 | 4.20 | 3.35 | β | 631 | β | β | β | β |
| Dias et al. | 2002 | 3.24 | 3.78 | β | 501 | β | β | β | β |

