Teutsch 144
(FSR 0297; MWSC 3500; DSH J2121.7+5036; FoF 510)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.8 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Teutsch 144 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 320.445 | 50.609 | 0.351 | -1.872 | -3.208 | -36.935 |
| Hu & Soubiran | 2025 | 320.461 | 50.602 | â | â | â | â |
| Almeida et al. | 2025 | 320.439 | 50.582 | â | â | â | â |
| Hunt & Reffert | 2024 | 320.435 | 50.614 | 0.349 | -1.863 | -3.224 | -34.744 |
| Cavallo et al. | 2024 | 320.461 | 50.602 | 0.35 | â | â | â |
| Hunt & Reffert | 2023 | 320.435 | 50.614 | 0.349 | -1.863 | -3.224 | -34.744 |
| Just et al. | 2023 | 320.418 | 50.593 | â | â | â | â |
| Dias et al. | 2021 | 320.439 | 50.582 | 0.345 | -1.909 | -3.126 | -33.296 |
| Cantat-Gaudin et al. | 2020 | 320.438 | 50.595 | 0.352 | -1.89 | -3.129 | â |
| Cantat-Gaudin & Anders | 2020 | 320.438 | 50.595 | 0.352 | -1.89 | -3.129 | â |
| Liu & Pang | 2019 | 320.474 | 50.571 | 0.351 | -1.891 | -3.063 | â |
| Soubiran et al. | 2018 | 320.438 | 50.595 | â | â | â | -32.0 |
| Bica et al. | 2019 | 320.427 | 50.607 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 320.438 | 50.595 | 0.352 | -1.89 | -3.129 | â |
| Loktin & Popova | 2017 | 320.415 | 50.593 | â | -0.498 | -0.286 | â |
| Kharchenko et al. | 2016 | 320.418 | 50.593 | â | â | â | â |
| Dias et al. | 2014 | 320.438 | 50.619 | â | -3.07 | -6.17 | â |
| Kharchenko et al. | 2013 | 320.422 | 50.597 | â | -1.88 | -1.0 | â |
| Kharchenko et al. | 2012 | 320.422 | 50.597 | â | -1.88 | -1.0 | â |
| Froebrich et al. | 2007 | 320.375 | 50.454 | â | â | â | â |
| Kronberger et al. | 2006 | 320.433 | 50.61 | â | â | â | â |
| Dias et al. | 2002 | 320.438 | 50.619 | â | -3.07 | -6.17 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.150* | â | â | â |
| Almeida et al. | 2025 | 2.14 | 2.40 | â | 448 | â | 471 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 801* | â | â |
| Cavallo et al. | 2024 | 2.58 | 2.32 | â | 562 | 0.580 | â | â | â |
| Hunt & Reffert | 2023 | 2.60 | 2.68 | 2.11 | 194 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 638 | â | 254 | â | â |
| Dias et al. | 2021 | 2.14 | 2.40 | â | 448 | 0.218 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.51 | 1.81 | â | 871 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.63 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1910 | -0.500 | â | â | â |
| Soubiran et al. | 2018 | 2.63 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.63 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.32 | 2.43 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.47 | 3.23 | â | 638 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.47 | 3.23 | â | 638 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.47 | 3.23 | â | 638 | â | â | â | â |
| Dias et al. | 2002 | 2.28 | 2.17 | â | 794 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.