Feibelman 1
(MWSC 3301)
0.85
UTI
0.6
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.7 [arcmin]
- CN 0.6 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Feibelman 1 is a moderately populated, very dense object of very 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, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Distant
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 | 304.427 | 38.03 | 0.258 | -3.2 | -4.99 | â |
| Li et al. | 2025 | 304.417 | 38.03 | 0.26 | -3.192 | -4.956 | â |
| Almeida et al. | 2025 | 304.428 | 38.029 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.421 | 38.03 | 0.253 | -3.192 | -4.991 | â |
| Cavallo et al. | 2024 | 304.424 | 38.023 | 0.254 | â | â | â |
| Hunt & Reffert | 2023 | 304.421 | 38.03 | 0.253 | -3.192 | -4.991 | â |
| Just et al. | 2023 | 304.441 | 38.03 | â | â | â | â |
| Dias et al. | 2021 | 304.428 | 38.029 | 0.249 | -3.212 | -4.953 | â |
| Cantat-Gaudin et al. | 2020 | 304.417 | 38.03 | 0.26 | -3.192 | -4.956 | â |
| Cantat-Gaudin & Anders | 2020 | 304.417 | 38.03 | 0.26 | -3.192 | -4.956 | â |
| Cantat-Gaudin et al. | 2018 | 304.417 | 38.03 | 0.26 | -3.192 | -4.956 | â |
| Loktin & Popova | 2017 | 304.44 | 38.033 | â | -0.504 | -0.464 | -8.9 |
| Kharchenko et al. | 2016 | 304.441 | 38.03 | â | â | â | â |
| Dias et al. | 2014 | 304.446 | 38.033 | â | -2.35 | -2.24 | -8.9 |
| Kharchenko et al. | 2013 | 304.446 | 38.033 | â | -1.52 | -0.96 | -8.9 |
| Dias et al. | 2002 | 304.446 | 38.033 | â | -2.35 | -2.24 | -8.9 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 3.04 | 1.98 | â | 424 | 0.035 | â | â | â |
| Almeida et al. | 2025 | 3.23 | 2.10 | â | 149 | â | 288 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 848* | â | â |
| Cavallo et al. | 2024 | 3.33 | 2.28 | â | 129 | 0.550 | â | â | â |
| Hunt & Reffert | 2023 | 3.43 | 2.46 | 1.90 | 17 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 5 | â | 26 | â | â |
| Dias et al. | 2021 | 3.23 | 2.10 | â | 149 | 0.140 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.94 | 1.93 | â | 138 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.46 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.46 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.37 | 0.64 | â | 871 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.46 | 6.58 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.46 | 6.58 | â | 5 | â | â | â | â |
| Dias et al. | 2002 | 1.46 | 6.58 | â | 5 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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