Teutsch 30
(MWSC 3345)
0.78
UTI
0.55
CN
1.0
Cdens
1.0
CC3
0.68
Clit
1.0
Cdup
Nm (P>50%)
60
Core radius and density
1.1 [pc], 5.5 [pc-2]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.68 Moderately studied
- Cdup 1.0 Unique
Overview
Teutsch 30 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 306.929 | 36.079 | 0.549 | -3.192 | -5.701 | 42.527 |
| Almeida et al. | 2025 | 306.929 | 36.078 | â | â | â | â |
| Hunt & Reffert | 2024 | 306.93 | 36.071 | 0.551 | -3.175 | -5.733 | 26.556 |
| Celli et al. | 2024 | 306.929 | 36.076 | â | â | â | â |
| Cavallo et al. | 2024 | 306.854 | 36.059 | 0.556 | â | â | â |
| Hunt & Reffert | 2023 | 306.93 | 36.071 | 0.551 | -3.175 | -5.733 | 26.556 |
| Just et al. | 2023 | 306.917 | 36.072 | â | â | â | â |
| Dias et al. | 2021 | 306.929 | 36.078 | 0.534 | -3.195 | -5.752 | â |
| Cantat-Gaudin et al. | 2020 | 306.929 | 36.074 | 0.539 | -3.18 | -5.692 | â |
| Cantat-Gaudin & Anders | 2020 | 306.929 | 36.074 | 0.539 | -3.18 | -5.692 | â |
| Dias et al. | 2019 | 306.929 | 36.076 | 0.534 | -3.172 | -5.682 | 94.08 |
| Soubiran et al. | 2018 | 306.929 | 36.074 | â | â | â | 94.08 |
| Cantat-Gaudin et al. | 2018 | 306.929 | 36.074 | 0.539 | -3.18 | -5.692 | â |
| Dias et al. | 2018 | â | â | â | -4.12 | -6.12 | â |
| Loktin & Popova | 2017 | 306.93 | 36.076 | â | 0.48 | -2.067 | â |
| Sampedro et al. | 2017 | 306.929 | 36.076 | â | â | â | â |
| Joshi et al. | 2016 | 306.922 | 36.075 | â | â | â | â |
| Kharchenko et al. | 2016 | 306.917 | 36.072 | â | â | â | â |
| Kharchenko et al. | 2013 | 306.922 | 36.075 | â | 0.14 | -5.11 | â |
| Bukowiecki et al. | 2011 | 306.925 | 36.071 | â | â | â | â |
| Kronberger et al. | 2006 | 306.929 | 36.076 | â | â | â | â |
| Dias et al. | 2002 | 306.929 | 36.076 | â | 1.34 | -6.55 | 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 | 1.76 | 3.48 | 2.72 | 29 | 0.161 | 241 | â | â |
| Almeida et al. | 2025 | 1.87 | 3.48 | â | 10 | â | 241 | â | â |
| Hunt & Reffert | 2024 | 1.70 | 3.54 | 2.72 | 21 | â | 682(1) | â | â |
| Celli et al. | 2024 | â | â | â | 29 | â | 217 | â | â |
| Cavallo et al. | 2024 | 1.93 | 3.70 | â | 46 | 0.650 | â | â | â |
| Hunt & Reffert | 2023 | 1.70 | 3.54 | 2.72 | 21 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 32 | â | 31 | â | â |
| Dias et al. | 2021 | 1.87 | 3.48 | â | 10 | -0.107 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.76 | 3.41 | â | 29 | â | â | â | â |
| Kounkel et al. | 2020 | 1.84 | 3.47 | â | 30 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.76 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 2.49 | 3.00 | â | 32 | 0.161 | â | â | â |
| Soubiran et al. | 2018 | 1.76 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.76 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.63 | 2.09 | â | 158 | â | â | â | â |
| Joshi et al. | 2016 | 1.38 | 2.96 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.38 | 2.96 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.38 | 2.96 | â | 32 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 266 | â | â |
| Bukowiecki et al. | 2011 | 2.37(1) | 4.01 | â | 11 | â | â | â | â |
| Kronberger et al. | 2006 | 1.60 | 3.91 | â | 8 | â | â | â | â |
| Dias et al. | 2002 | 1.60 | 3.91 | â | 8 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2833, e_all=0.0356.