ASCC 65
(MWSC 1909)
0.75
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
13.0 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 65 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 an extremely massive, near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 167.825 | -61.123 | 0.384 | -6.289 | 1.145 | 3.006 |
| Liu et al. | 2025 | 167.83 | -61.17 | 0.38 | -6.31 | 1.13 | 4.17 |
| Hunt & Reffert | 2024 | 167.834 | -61.167 | 0.382 | -6.309 | 1.133 | 4.172 |
| Cavallo et al. | 2024 | 167.869 | -61.144 | 0.385 | â | â | â |
| Hunt & Reffert | 2023 | 167.834 | -61.167 | 0.382 | -6.309 | 1.133 | 4.172 |
| Bica et al. | 2019 | 167.765 | -61.117 | â | â | â | â |
| Dias et al. | 2014 | 167.775 | -61.12 | â | -3.48 | -2.27 | â |
| Gozha et al. | 2012 | 167.775 | -61.12 | â | â | â | â |
| Piskunov et al. | 2008 | 167.765 | -61.117 | â | â | â | â |
| Kharchenko et al. | 2007 | 167.77 | -61.12 | â | 0.22 | â | -13.4 |
| Kharchenko et al. | 2005 | 167.77 | -61.12 | â | -6.83 | 0.88 | -13.4 |
| Dias et al. | 2002 | 167.775 | -61.12 | â | -3.48 | -2.27 | -14.39 |
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 | 3.5 | 1.24 | 1.93 | 12 | -0.070 | 14624 | â | â |
| Liu et al. | 2025 | 3.39 | 0.43 | â | 7 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 408(1) | â | â |
| Cavallo et al. | 2024 | 2.13 | 1.32 | â | 13 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.36 | 1.09 | 1.93 | 6 | â | â | â | â |
| Gozha et al. | 2012 | 3.50 | â | â | 12 | â | 28840 | â | â |
| Piskunov et al. | 2008 | 3.50 | 1.24 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 3.50 | 1.24 | â | 12 | â | â | â | â |
| Dias et al. | 2002 | 3.50 | 1.24 | â | 12 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 10 along with HSC_2406, and of multiple system 6 along with HSC_2406 and NGC_3590.
Palma et al. (2025)
Part of multiple system G154, along with NGC_3590, NGC_3572, HSC_2406 and UBC_659.
Cavallo et al. (2024)
Silver sample.