ASCC 125
(FSR 0409; MWSC 3677)
0.77
UTI
0.85
CN
1.0
Cdens
0.75
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
423.5 [N/pc2]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 125 is a rich, very dense object of high C3 quality. Its parallax locates it at a close* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~0.84 kpc) differs significantly from the median photometric distance (~1.50 kpc).
Note: This object shares a significant percentage of members with 2 later reported entries. 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 | 99999â | 344.112 | 62.711 | 1.187 | -0.539 | -2.179 | -24.599 |
| Wei et al. | 2025 | 344.153 | 62.754 | 1.176 | -1.151 | -2.386 | â |
| Hunt & Reffert | 2024 | 344.102 | 62.711 | 1.191 | -0.541 | -2.197 | -23.131 |
| Cavallo et al. | 2024 | 344.084 | 62.698 | 1.185 | â | â | â |
| Hunt & Reffert | 2023 | 344.102 | 62.711 | 1.191 | -0.541 | -2.197 | -23.131 |
| Bica et al. | 2019 | 344.079 | 62.746 | â | â | â | â |
| Dias et al. | 2014 | 344.071 | 62.75 | â | -0.66 | -1.47 | â |
| Gozha et al. | 2012 | 344.071 | 62.75 | â | â | â | â |
| Piskunov et al. | 2008 | 344.059 | 62.742 | â | â | â | â |
| Kharchenko et al. | 2007 | 344.07 | 62.75 | â | 0.55 | â | -17.93 |
| Kharchenko et al. | 2005 | 344.07 | 62.75 | â | -2.23 | -3.44 | -17.93 |
| Dias et al. | 2002 | 344.071 | 62.75 | â | -0.66 | -1.47 | -20.52 |
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 | 1.5 | 2.585 | 2.45 | 10 | -0.265 | 4913 | 0.52 | â |
| Wei et al. | 2025 | 1.22 | 2.97 | â | 15 | -0.750 | 4913 | 0.52 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 316(1) | â | â |
| Cavallo et al. | 2024 | 1.11 | 3.01 | â | 6 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 0.82 | 3.83 | 2.45 | 4 | â | â | â | â |
| Gozha et al. | 2012 | 1.50 | â | â | 10 | â | 29512 | â | â |
| Piskunov et al. | 2008 | 1.50 | 2.20 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.50 | 2.20 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 2.20 | â | 10 | 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)
Bronze sample.