Teutsch 110
(DSH J1326.5-6406)
0.47
UTI
0.52
CN
0.58
Cdens
1.0
CC3
0.13
Clit
1.0
Cdup
Nm (P>50%)
55
Core radius and density
1.9 [pc], 2.9 [pc-2]
- CN 0.52 Moderately populated
- Cdens 0.58 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.13 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
Teutsch 110 is a moderately populated, moderately 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 rarely studied in the literature.
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 | 6.27 | 2.94 | 1.88 | 259 | -0.710 | 1867 | â | â |
| Hunt & Reffert | 2024 | 6.27 | 2.94 | 1.88 | 259 | 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.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.76 (50th percentile), true positive? (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.76 (50th percentile), true positive? (human-assigned).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.