Teutsch J0924.3-5313
0.28
UTI
0.35
CN
0.67
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
35
Core radius and density
1.0 [pc], 3.3 [pc-2]
- CN 0.35 Poorly populated
- Cdens 0.67 Moderately dense
- CC3 0.25 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Teutsch J0924.3-5313 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (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 | 141.099 | -53.218 | 0.175 | -4.312 | 3.927 | 60.524 |
| Hunt & Reffert | 2024 | 141.091 | -53.214 | 0.174 | -4.286 | 3.943 | â |
| Cavallo et al. | 2024 | 141.099 | -53.217 | 0.176 | â | â | â |
| Hunt & Reffert | 2023 | 141.091 | -53.214 | 0.174 | -4.286 | 3.943 | â |
| Bica et al. | 2019 | 141.096 | -53.221 | 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 | 5.32 | 2.69 | 1.9 | 78 | 0.020 | 690 | â | â |
| Hunt & Reffert | 2024 | 5.32 | 2.69 | 1.90 | 78 | â | 690(1) | â | â |
| Cavallo et al. | 2024 | 2.87 | 2.63 | â | 347 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 5.32 | 2.69 | 1.90 | 78 | 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 classes: 0.07 (50th percentile), false positive? (human-assigned).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.