Moffat 1
(MWSC 2346; C1557-540)
0.81
UTI
0.38
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.38 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Moffat 1 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Metal-rich
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 240.403 | -54.144 | 0.402 | -2.294 | -3.029 | -49.562 |
| Almeida et al. | 2025 | 240.41 | -54.151 | â | â | â | â |
| Hunt & Reffert | 2024 | 240.399 | -54.146 | 0.396 | -2.318 | -3.019 | -51.7 |
| Cavallo et al. | 2024 | 240.403 | -54.146 | 0.401 | â | â | â |
| Hunt & Reffert | 2023 | 240.399 | -54.146 | 0.396 | -2.318 | -3.019 | -51.7 |
| Just et al. | 2023 | 240.363 | -54.116 | â | â | â | â |
| Dias et al. | 2021 | 240.41 | -54.151 | 0.404 | -2.225 | -3.018 | â |
| Cantat-Gaudin et al. | 2020 | 240.397 | -54.149 | 0.402 | -2.211 | -3.037 | â |
| Cantat-Gaudin & Anders | 2020 | 240.397 | -54.149 | 0.402 | -2.211 | -3.037 | â |
| Bica et al. | 2019 | 240.399 | -54.143 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 240.397 | -54.149 | 0.402 | -2.211 | -3.037 | â |
| Kharchenko et al. | 2016 | 240.363 | -54.116 | â | â | â | â |
| Dias et al. | 2014 | 240.375 | -54.117 | â | -3.8 | -4.41 | -42.0 |
| Kharchenko et al. | 2013 | 240.375 | -54.117 | â | 0.52 | -0.76 | -42.0 |
| van den Bergh | 2006 | 240.375 | -54.133 | â | â | â | â |
| Dias et al. | 2002 | 240.375 | -54.117 | â | -3.8 | -4.41 | -42.0 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.51 | 2.41 | â | 6 | â | 112 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 941* | â | â |
| Cavallo et al. | 2024 | 1.76 | 2.00 | â | 32 | 0.520 | â | â | â |
| Hunt & Reffert | 2023 | 2.27 | 2.99 | 2.61 | 16 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 6 | â | 90 | â | â |
| Dias et al. | 2021 | 2.51 | 2.41 | â | 6 | 0.500 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.28 | 2.02 | â | 78 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.32 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.32 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.12 | 2.90 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.12 | 2.90 | â | 6 | â | â | â | â |
| van den Bergh | 2006 | 3.30 | 5.70 | â | 4 | â | â | â | â |
| Dias et al. | 2002 | 2.10 | 3.10 | â | 10 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Silver sample.