Teutsch 330
0.29
UTI
0.33
CN
0.14
Cdens
0.75
CC3
0.12
Clit
1.0
Cdup
Nm (P>50%)
33
Core radius and density
2.8 [pc], 0.7 [pc-2]
- CN 0.33 Poorly populated
- Cdens 0.14 Very loose
- CC3 0.75 High quality
- Clit 0.12 Rarely studied
- Cdup 1.0 Unique
Overview
Teutsch 330 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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 | 338.894 | 56.204 | 0.229 | -3.501 | -2.81 | â |
| Hunt & Reffert | 2024 | 338.918 | 56.202 | 0.237 | -3.501 | -2.802 | â |
| Cavallo et al. | 2024 | 338.883 | 56.186 | 0.234 | â | â | â |
| Hunt & Reffert | 2023 | 338.918 | 56.202 | 0.237 | -3.501 | -2.802 | â |
| Bica et al. | 2019 | 338.92 | 56.205 | 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 | 3.92 | 2.07 | 0.98 | 108 | -0.260 | 431 | â | â |
| Hunt & Reffert | 2024 | 3.92 | 2.07 | 0.98 | 108 | â | 431(1) | â | â |
| Cavallo et al. | 2024 | 3.37 | 2.26 | â | 25 | -0.260 | â | â | â |
| Hunt & Reffert | 2023 | 3.92 | 2.07 | 0.98 | 108 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.