Teutsch 23
(MWSC 3760; DSH J2347.9+6259; FSR 0454)
0.84
UTI
0.75
CN
0.71
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
3.5 [N/pc2]
- CN 0.75 Rich
- Cdens 0.71 Moderately dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Teutsch 23 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the distance, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. 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 | 99999β | 356.947 | 63.048 | 0.31 | -2.969 | -1.402 | -66.908 |
| Almeida et al. | 2025 | 356.986 | 63.002 | β | β | β | β |
| Hunt & Reffert | 2024 | 356.968 | 62.993 | 0.317 | -2.952 | -1.425 | β |
| Celli et al. | 2024 | 356.976 | 62.997 | β | β | β | β |
| Cavallo et al. | 2024 | 356.946 | 62.992 | 0.317 | β | β | β |
| Hunt & Reffert | 2023 | 356.968 | 62.993 | 0.317 | -2.952 | -1.425 | β |
| Just et al. | 2023 | 356.954 | 62.993 | β | β | β | β |
| Dias et al. | 2021 | 356.986 | 63.002 | 0.283 | -2.978 | -1.413 | β |
| Cantat-Gaudin et al. | 2020 | 356.976 | 62.996 | 0.29 | -2.986 | -1.387 | β |
| SΓ‘nchez et al. | 2020 | 356.979 | 62.99 | β | -3.05 | -1.317 | β |
| Cantat-Gaudin & Anders | 2020 | 356.976 | 62.996 | 0.29 | -2.986 | -1.387 | β |
| Soubiran et al. | 2018 | 356.976 | 62.996 | β | β | β | 77.45 |
| Bica et al. | 2019 | 356.97 | 62.997 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 356.976 | 62.996 | 0.29 | -2.986 | -1.387 | β |
| Loktin & Popova | 2017 | 356.985 | 62.99 | β | 2.556 | -5.789 | β |
| Kharchenko et al. | 2016 | 356.954 | 62.993 | β | β | β | β |
| Dias et al. | 2014 | 356.979 | 62.99 | β | 0.1 | -2.15 | β |
| Kharchenko et al. | 2013 | 356.962 | 62.997 | β | 3.66 | -5.83 | β |
| Kharchenko et al. | 2012 | 356.962 | 62.997 | β | 3.66 | -5.83 | β |
| Bukowiecki et al. | 2011 | 356.979 | 62.999 | β | β | β | β |
| Kronberger et al. | 2006 | 356.976 | 62.997 | β | β | β | β |
| Dias et al. | 2002 | 356.979 | 62.99 | β | 0.1 | -2.15 | β |
π‘ 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 | 99999β | 2.8 | 2.39 | 0.43 | 13 | 0.236 | 371 | β | β |
| Liu et al. | 2025 | 9.38 | 1.09 | β | 10 | β | β | β | β |
| Almeida et al. | 2025 | 2.64 | 2.85 | β | 12 | β | 157 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 371(1) | β | β |
| Celli et al. | 2024 | β | β | β | 6 | β | 537 | β | β |
| Cavallo et al. | 2024 | 3.40 | 3.05 | β | 21 | 0.560 | β | β | β |
| Hunt & Reffert | 2023 | 3.00 | 3.31 | 0.43 | 13 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 13 | β | 44 | β | β |
| Dias et al. | 2021 | 2.64 | 2.85 | β | 12 | -0.088 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.45 | 2.69 | β | 6 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.14 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.14 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.14 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.32 | 2.04 | β | 65 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.80 | 2.39 | β | 13 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.80 | 2.39 | β | 13 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 455 | β | β |
| Kharchenko et al. | 2012 | 2.80 | 2.39 | β | 13 | β | β | β | β |
| Bukowiecki et al. | 2011 | 2.70(1) | 2.26 | β | 13 | β | β | β | β |
| Dias et al. | 2002 | 2.68 | 2.39 | β | 10 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 270 along with King_21.
Palma et al. (2025)
Classified as optical pair P60, along with King_21.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.