Teutsch 118
(FSR 0111; DSH J1908.1+0414)
0.06
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.09
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 0.09 Very likely duplicate
Overview
Teutsch 118 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
(*): The parallax distance estimate (~3.64 kpc) differs significantly from the median photometric distance (~2.77 kpc).
Relatively close
High extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 286.923 | 4.343 | 0.275 | -1.584 | -4.71 | 46.549 |
| Hunt & Reffert | 2024 | 286.924 | 4.344 | 0.281 | -1.587 | -4.683 | 35.109 |
| Cavallo et al. | 2024 | 286.914 | 4.329 | 0.278 | â | â | â |
| Hunt & Reffert | 2023 | 286.924 | 4.344 | 0.281 | -1.587 | -4.683 | 35.109 |
| Bica et al. | 2019 | 286.932 | 4.348 | â | â | â | â |
| Kronberger et al. | 2006 | 287.038 | 4.233 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1982* | â | â |
| Cavallo et al. | 2024 | 2.43 | 2.98 | â | 389 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 3.11 | 3.20 | 2.08 | 124 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.