ASCC 79
(MWSC 2288; Alessi 25)
0.91
UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
13.5 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
ASCC 79 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a significant percentage of members with 3 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 | 229.731 | -60.931 | 1.183 | -3.046 | -4.131 | -7.27 |
| Almeida et al. | 2025 | 229.686 | -60.806 | â | â | â | â |
| Alfonso et al. | 2024 | 229.822 | -60.815 | 1.143 | -3.027 | -3.968 | â |
| Hunt & Reffert | 2024 | 229.367 | -61.075 | 1.187 | -3.069 | -4.0 | -8.86 |
| Celli et al. | 2024 | 229.731 | -60.798 | â | â | â | â |
| Cavallo et al. | 2024 | 229.781 | -60.83 | 1.185 | â | â | â |
| Hunt & Reffert | 2023 | 229.367 | -61.075 | 1.187 | -3.069 | -4.0 | -8.86 |
| Just et al. | 2023 | 229.652 | -60.628 | â | â | â | â |
| He et al. | 2022 | 229.708 | -60.912 | 1.184 | -3.109 | -4.106 | â |
| Dias et al. | 2021 | 229.686 | -60.806 | 1.178 | -2.942 | -4.214 | 12.322 |
| Cantat-Gaudin et al. | 2020 | 229.731 | -60.798 | 1.176 | -2.914 | -4.232 | â |
| Cantat-Gaudin & Anders | 2020 | 229.731 | -60.798 | 1.176 | -2.914 | -4.232 | â |
| Dias et al. | 2019 | 229.729 | -60.798 | 1.176 | -2.914 | -4.232 | -4.619 |
| Soubiran et al. | 2018 | 229.731 | -60.798 | â | â | â | -1.4 |
| Bica et al. | 2019 | 229.792 | -60.727 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 229.731 | -60.798 | 1.176 | -2.914 | -4.232 | â |
| Kharchenko et al. | 2016 | 229.652 | -60.628 | â | â | â | â |
| Dias et al. | 2014 | 229.8 | -60.73 | â | -4.81 | -4.57 | â |
| Kharchenko et al. | 2013 | 229.665 | -60.63 | â | -3.55 | -4.2 | 4.5 |
| Gozha et al. | 2012 | 229.8 | -60.73 | â | â | â | â |
| Piskunov et al. | 2008 | 229.792 | -60.727 | â | â | â | â |
| Kharchenko et al. | 2007 | 229.8 | -60.73 | â | 0.52 | â | 4.53 |
| Kharchenko et al. | 2005 | 229.8 | -60.73 | â | -2.67 | -4.1 | 4.03 |
| Dias et al. | 2002 | 229.8 | -60.73 | â | -2.67 | -4.1 | -1.01 |
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 | 0.825 | 0.62 | 1.75 | 9 | -0.073 | 671 | â | â |
| Almeida et al. | 2025 | 0.83 | 0.75 | â | 23 | â | 726 | â | â |
| Alfonso et al. | 2024 | 0.77 | 0.41 | â | 12 | 0.048 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 240(1) | â | â |
| Celli et al. | 2024 | â | â | â | 19 | â | 671 | â | â |
| Cavallo et al. | 2024 | 0.84 | 0.87 | â | 3 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.80 | 0.62 | 1.75 | 5 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 9 | â | 485 | â | â |
| He et al. | 2022 | â | 1.00 | â | 5 | â | â | â | â |
| Dias et al. | 2021 | 0.83 | 0.75 | â | 23 | 0.043 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.82 | 0.41 | â | 19 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.83 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 0.81 | 0.59 | â | 9 | -0.775 | â | â | â |
| Soubiran et al. | 2018 | 0.83 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.83 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 0.87 | 0.97 | â | 9 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.87 | 0.97 | â | 9 | â | â | â | â |
| Gozha et al. | 2012 | 0.80 | â | â | 7 | â | 2344 | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.50 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.50 | â | 7 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.50 | â | 7 | 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.