Teutsch 27
(MWSC 3144; DSH J1937.3+1841)
0.67
UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
107.2 [N/pc2]
- CN 0.33 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Teutsch 27 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 294.343 | 18.7 | 0.262 | -2.949 | -6.321 | 34.984 |
| Hunt & Reffert | 2024 | 294.344 | 18.701 | 0.247 | -2.959 | -6.342 | â |
| Cavallo et al. | 2024 | 294.326 | 18.696 | 0.25 | â | â | â |
| Hunt & Reffert | 2023 | 294.344 | 18.701 | 0.247 | -2.959 | -6.342 | â |
| Just et al. | 2023 | 294.336 | 18.692 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 294.343 | 18.7 | 0.245 | -2.924 | -6.308 | â |
| Cantat-Gaudin & Anders | 2020 | 294.343 | 18.7 | 0.245 | -2.924 | -6.308 | â |
| Bica et al. | 2019 | 294.341 | 18.696 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 294.343 | 18.7 | 0.245 | -2.924 | -6.308 | â |
| Loktin & Popova | 2017 | 294.345 | 18.715 | â | 1.9 | -3.625 | â |
| Kharchenko et al. | 2016 | 294.336 | 18.692 | â | â | â | â |
| Kharchenko et al. | 2013 | 294.342 | 18.695 | â | 1.08 | -4.51 | â |
| Morales et al. | 2013 | 294.346 | 18.699 | â | â | â | â |
| Kronberger et al. | 2006 | 294.347 | 18.697 | â | â | â | â |
| Dias et al. | 2002 | 294.346 | 18.699 | â | -1.76 | -5.0 | 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 | 3.625 | 3.07 | 1.83 | 562 | 0.640 | 690 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 581(1) | â | â |
| Cavallo et al. | 2024 | 4.15 | 3.35 | â | 7 | 0.640 | â | â | â |
| Hunt & Reffert | 2023 | 3.38 | 3.43 | 1.83 | 8 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 562 | â | 798 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.31 | 3.03 | â | 32 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.65 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 4.21 | 2.50 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.60 | 3.07 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.60 | 3.07 | â | 562 | â | â | â | â |
| Morales et al. | 2013 | 2.48 | â | â | 600 | â | â | â | â |
| Dias et al. | 2002 | 2.48 | 2.98 | â | 603 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.
Cavallo et al. (2024)
Gold sample.