ASCC 113
(MWSC 3480; FoF 2406)
0.97
UTI
0.87
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
12.7 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
ASCC 113 is a rich, very dense object of very 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, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. 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 | 317.985 | 38.681 | 1.767 | 0.823 | -3.71 | -5.559 |
| Li et al. | 2025 | 317.933 | 38.638 | 1.762 | 0.8 | -3.679 | â |
| Wei et al. | 2025 | 317.986 | 38.623 | 1.764 | 0.824 | -3.746 | â |
| Almeida et al. | 2025 | 318.093 | 38.586 | â | â | â | â |
| Alfonso et al. | 2024 | 318.031 | 38.782 | 1.741 | 0.831 | -3.706 | â |
| Zhang et al. | 2024 | 317.963 | 38.545 | â | â | â | â |
| Hunt & Reffert | 2024 | 317.963 | 38.545 | 1.771 | 0.828 | -3.686 | -6.493 |
| Cavallo et al. | 2024 | 317.998 | 38.797 | 1.769 | â | â | â |
| Hunt & Reffert | 2023 | 317.963 | 38.545 | 1.771 | 0.828 | -3.686 | -6.493 |
| Almeida et al. | 2023 | 318.009 | 38.641 | â | â | â | â |
| Just et al. | 2023 | 318.002 | 38.607 | â | â | â | â |
| He et al. | 2022 | 317.955 | 38.656 | 1.767 | 0.809 | -3.724 | â |
| Tarricq et al. | 2022 | 317.926 | 38.543 | 1.768 | 0.826 | -3.708 | â |
| Dias et al. | 2021 | 318.093 | 38.586 | 1.762 | 0.798 | -3.688 | -4.195 |
| Cantat-Gaudin et al. | 2020 | 317.933 | 38.638 | 1.762 | 0.8 | -3.679 | â |
| Cantat-Gaudin & Anders | 2020 | 317.933 | 38.638 | 1.762 | 0.8 | -3.679 | â |
| Liu & Pang | 2019 | 318.043 | 38.763 | 1.774 | 0.78 | -3.652 | â |
| Bossini et al. | 2019 | 317.933 | 38.638 | â | â | â | â |
| Soubiran et al. | 2018 | 317.933 | 38.638 | â | â | â | -4.44 |
| Bica et al. | 2019 | 317.992 | 38.599 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 317.933 | 38.638 | 1.762 | 0.8 | -3.679 | â |
| Kharchenko et al. | 2016 | 318.002 | 38.607 | â | â | â | â |
| Dias et al. | 2014 | 318.0 | 38.6 | â | -1.78 | -4.19 | â |
| Kharchenko et al. | 2013 | 318.007 | 38.61 | â | 0.4 | -4.95 | â |
| Piskunov et al. | 2008 | 317.993 | 38.599 | â | â | â | â |
| Kharchenko et al. | 2005 | 318.0 | 38.6 | â | 1.04 | -4.22 | â |
| Dias et al. | 2002 | 318.0 | 38.6 | â | 1.04 | -4.22 | â |
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 | 0.56 | 0.12 | 0.48 | 138 | 0.000 | 413 | 0.4 | â |
| Li et al. | 2025 | 0.60 | 0.02 | â | 379 | 0.340 | â | â | â |
| Wei et al. | 2025 | 0.58 | 0.33 | â | 135 | 0.250 | 451 | 0.39 | â |
| Almeida et al. | 2025 | 0.56 | 0.28 | â | 285 | â | 156 | â | â |
| Alfonso et al. | 2024 | 0.56 | 0.13 | â | 432 | -0.051 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.073(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 609(1) | â | â |
| Cavallo et al. | 2024 | 0.56 | 0.36 | â | 132 | 0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.54 | 0.11 | 0.48 | 184 | â | â | â | â |
| Almeida et al. | 2023 | 0.56 | 0.24 | â | 311 | 0.001 | 413(1) | 0.41 | â |
| Just et al. | 2023 | â | â | â | 85 | â | 29 | â | â |
| He et al. | 2022 | â | 0.35 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.56 | â | â | 302 | â | â | â | â |
| Dias et al. | 2021 | 0.56 | 0.28 | â | 285 | -0.052 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.56 | 0.13 | â | 288 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.56 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 65 | -0.250 | â | â | â |
| Bossini et al. | 2019 | 0.53 | 0.09 | â | 426 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.56 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.56 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 0.50 | 0.00 | â | 85 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.50 | 0.00 | â | 85 | â | â | â | â |
| Piskunov et al. | 2008 | 0.45 | 0.00 | â | 138 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.45 | 0.00 | â | 138 | â | â | â | â |
| Dias et al. | 2002 | 0.45 | 0.00 | â | 138 | 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: good fit.
Cavallo et al. (2024)
Gold sample.