Teutsch 44
(DSH J1021.4-5427; FSR 1528; MWSC 1795)
0.69
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Nm (P>50%)
228
Core radius and density
1.2 [pc], 7.0 [pc-2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
Teutsch 44 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 155.347 | -54.447 | 0.128 | -4.592 | 2.277 | 55.962 |
| Hu & Soubiran | 2025 | 155.369 | -54.45 | â | â | â | â |
| Hunt & Reffert | 2024 | 155.348 | -54.449 | 0.138 | -4.585 | 2.307 | 57.36 |
| Cavallo et al. | 2024 | 155.369 | -54.45 | 0.133 | â | â | â |
| Hunt & Reffert | 2023 | 155.348 | -54.449 | 0.138 | -4.585 | 2.307 | 57.36 |
| Jadhav & Subramaniam | 2021 | 155.347 | -54.45 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 155.347 | -54.45 | 0.1 | -4.613 | 2.239 | â |
| Cantat-Gaudin & Anders | 2020 | 155.347 | -54.45 | 0.1 | -4.613 | 2.239 | â |
| Soubiran et al. | 2018 | 155.347 | -54.45 | â | â | â | 57.67 |
| Bica et al. | 2019 | 155.345 | -54.451 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 155.347 | -54.45 | 0.1 | -4.613 | 2.239 | â |
| Dias et al. | 2018 | â | â | â | -6.02 | 1.01 | â |
| Sampedro et al. | 2017 | 155.35 | -54.451 | â | -3.24 | 0.81 | â |
| Dias et al. | 2014 | 155.35 | -54.451 | â | -3.15 | -0.58 | â |
| Kronberger et al. | 2006 | 155.352 | -54.451 | â | â | â | â |
| Dias et al. | 2002 | 155.35 | -54.451 | â | -3.15 | -0.58 | 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 | 6.95 | 1.73 | 1.99 | 1259 | -0.315 | 1252 | â | 1 |
| Hu & Soubiran | 2025 | â | â | â | â | -0.220(5) | â | â | â |
| Hunt & Reffert | 2024 | 6.70 | 1.76 | 1.99 | 1171 | â | 1497(1) | â | â |
| Cavallo et al. | 2024 | 5.89 | 1.73 | â | 1622 | -0.410 | â | â | â |
| Hunt & Reffert | 2023 | 6.70 | 1.76 | 1.99 | 1172 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 6.95 | 0.58 | â | 2570 | â | 1008 | â | 1(1) |
| Cantat-Gaudin et al. | 2020 | 6.95 | 0.58 | â | 2570 | â | â | â | â |
| Kounkel et al. | 2020 | 5.62 | 1.48 | â | 1259 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.74 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.74 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.74 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 7.41 | 2.02 | â | 692 | 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 class: 0.12 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.12 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0414, e_all=0.1273.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).