ASCC 9
(MWSC 228)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
6.4 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
ASCC 9 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 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 very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 41.704 | 57.735 | 0.401 | 0.162 | -1.125 | -48.277 |
| Almeida et al. | 2025 | 41.679 | 57.763 | â | â | â | â |
| Hunt & Reffert | 2024 | 41.624 | 57.777 | 0.402 | 0.169 | -1.139 | -23.791 |
| Celli et al. | 2024 | 41.671 | 57.743 | â | â | â | â |
| Cavallo et al. | 2024 | 41.691 | 57.735 | 0.402 | â | â | â |
| Hunt & Reffert | 2023 | 41.624 | 57.777 | 0.402 | 0.169 | -1.139 | -23.791 |
| Almeida et al. | 2023 | 41.696 | 57.783 | â | â | â | â |
| Just et al. | 2023 | 41.733 | 57.743 | â | â | â | â |
| Dias et al. | 2021 | 41.679 | 57.763 | 0.409 | 0.16 | -1.105 | â |
| Cantat-Gaudin et al. | 2020 | 41.671 | 57.743 | 0.406 | 0.166 | -1.099 | â |
| Cantat-Gaudin & Anders | 2020 | 41.671 | 57.743 | 0.406 | 0.166 | -1.099 | â |
| Dias et al. | 2019 | 41.729 | 57.73 | 0.391 | 0.156 | -1.086 | -72.118 |
| Cantat-Gaudin et al. | 2018 | 41.671 | 57.743 | 0.406 | 0.166 | -1.099 | â |
| Kharchenko et al. | 2016 | 41.733 | 57.743 | â | â | â | â |
| Dias et al. | 2014 | 41.729 | 57.73 | â | -0.93 | -0.33 | â |
| Kharchenko et al. | 2013 | 41.745 | 57.745 | â | -0.32 | -2.5 | -41.8 |
| Gozha et al. | 2012 | 41.729 | 57.73 | â | â | â | â |
| Kharchenko et al. | 2012 | 41.745 | 57.745 | â | -0.41 | -2.54 | -41.75 |
| Piskunov et al. | 2008 | 41.71 | 57.726 | â | â | â | â |
| Kharchenko et al. | 2007 | 41.73 | 57.73 | â | 0.17 | â | -41.75 |
| Kharchenko et al. | 2005 | 41.73 | 57.73 | â | 0.76 | -3.03 | -41.75 |
| Dias et al. | 2002 | 41.729 | 57.73 | â | -0.93 | -0.33 | -40.73 |
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 | 2.61 | 2.58 | 1.08 | 10 | -0.133 | 1010 | 0.58 | â |
| Almeida et al. | 2025 | 2.32 | 2.57 | â | 9 | â | 645 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1143(1) | â | â |
| Celli et al. | 2024 | â | â | â | 30 | â | 595 | â | â |
| Cavallo et al. | 2024 | 2.84 | 2.54 | â | 23 | 0.630 | â | â | â |
| Hunt & Reffert | 2023 | 2.34 | 2.50 | 1.08 | 29 | â | â | â | â |
| Almeida et al. | 2023 | 2.12 | 2.58 | â | 18 | -0.106 | 2154(1) | 0.58 | â |
| Just et al. | 2023 | â | â | â | 10 | â | 877 | â | â |
| Dias et al. | 2021 | 2.32 | 2.57 | â | 9 | -0.159 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.38 | 2.23 | â | 30 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.30 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 2.05 | 2.51 | â | 19 | -2.028 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.30 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.90 | 2.79 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.90 | 2.79 | â | 10 | â | â | â | â |
| Gozha et al. | 2012 | 2.90 | â | â | 6 | â | 2951 | â | â |
| Kharchenko et al. | 2012 | 2.90 | 2.79 | â | 10 | â | â | â | â |
| Piskunov et al. | 2008 | 2.90 | 2.79 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.90 | 2.79 | â | 6 | â | â | â | â |
| Dias et al. | 2002 | 2.90 | 2.79 | â | 6 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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