Teutsch 110
(DSH J1326.5-6406)
0.64
UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
17.5 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch 110 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.78 kpc) differs significantly from the median photometric distance (~5.13 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 201.638 | -64.103 | 0.147 | -6.955 | -1.365 | -43.877 |
| Hunt & Reffert | 2024 | 201.637 | -64.106 | 0.138 | -6.96 | -1.376 | -40.992 |
| Cavallo et al. | 2024 | 201.635 | -64.1 | 0.138 | â | â | â |
| Hunt & Reffert | 2023 | 201.637 | -64.106 | 0.138 | -6.96 | -1.376 | -40.992 |
| Bica et al. | 2019 | 201.648 | -64.1 | â | â | â | â |
| Morales et al. | 2013 | 201.649 | -64.103 | â | â | â | â |
| Kronberger et al. | 2006 | 201.649 | -64.103 | â | â | â | 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 | 5.135 | 3.0 | 1.88 | 364 | -0.710 | 1867 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1867(1) | â | â |
| Cavallo et al. | 2024 | 4.00 | 3.06 | â | 468 | -0.710 | â | â | â |
| Hunt & Reffert | 2023 | 6.27 | 2.94 | 1.88 | 259 | 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.