Teutsch 39
(MWSC 3643; Teutsch J2236.4+3747)
0.84
UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
28.6 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 39 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with 4 later reported entries. See table with shared members information.
Close
Low extinction
Low mass
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 339.215 | 37.764 | 2.04 | -1.763 | -6.045 | -13.077 |
| Zhang et al. | 2024 | 339.124 | 37.771 | â | â | â | â |
| Cavallo et al. | 2024 | 339.495 | 37.605 | 2.01 | â | â | â |
| Hunt & Reffert | 2023 | 339.124 | 37.771 | 2.011 | -1.6 | -6.122 | -13.143 |
| Just et al. | 2023 | 339.148 | 37.722 | â | â | â | â |
| He et al. | 2022 | 340.792 | 40.065 | 2.303 | -2.014 | -5.261 | â |
| Bica et al. | 2019 | 339.12 | 37.784 | â | â | â | â |
| Loktin & Popova | 2017 | 339.12 | 37.756 | â | -2.794 | -5.011 | -19.5 |
| Kharchenko et al. | 2016 | 339.148 | 37.722 | â | â | â | â |
| Dias et al. | 2014 | 339.121 | 37.756 | â | -2.97 | -2.38 | â |
| Kharchenko et al. | 2013 | 339.154 | 37.726 | â | -4.37 | -6.15 | -19.5 |
| Kharchenko et al. | 2012 | 339.154 | 37.726 | â | -4.37 | -6.15 | -19.5 |
| Dias et al. | 2002 | 339.121 | 37.756 | â | -3.25 | -2.32 | -19.5 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.130* | â | â | â |
| Cavallo et al. | 2024 | 0.53 | 0.69 | â | 8 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 0.48 | 0.27 | 0.56 | 15 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 50 | â | 6 | â | â |
| He et al. | 2022 | â | 0.10 | â | 11 | â | â | â | â |
| Loktin & Popova | 2017 | 0.79 | 0.86 | â | 603 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.60 | 0.62 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.60 | 0.62 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2012 | 0.60 | 0.62 | â | 50 | â | â | â | â |
| Dias et al. | 2002 | 0.81 | 0.25 | â | 20 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.