Teutsch 324
0.20
UTI
0.29
CN
0.09
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
29
Core radius and density
2.6 [pc], 0.5 [pc-2]
- CN 0.29 Poorly populated
- Cdens 0.09 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Teutsch 324 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 327.949 | 56.709 | 0.132 | -2.847 | -2.244 | â |
| Hunt & Reffert | 2024 | 327.942 | 56.711 | 0.137 | -2.804 | -2.23 | -10.5 |
| Cavallo et al. | 2024 | 328.096 | 56.686 | 0.131 | â | â | â |
| Hunt & Reffert | 2023 | 327.942 | 56.711 | 0.137 | -2.804 | -2.23 | -10.5 |
| Bica et al. | 2019 | 327.935 | 56.707 | 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 | 7.14 | 4.17 | 2.64 | 9 | 0.500 | 893 | â | â |
| Hunt & Reffert | 2024 | 7.14 | 4.17 | 2.64 | 9 | â | 893(1) | â | â |
| Cavallo et al. | 2024 | 4.49 | 3.81 | â | 22 | 0.500 | â | â | â |
| Hunt & Reffert | 2023 | 7.14 | 4.17 | 2.64 | 9 | 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)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.10 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.10 (50th percentile).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.