ASCC 113
(MWSC 3480; FoF 2406)
- 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. 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 | – | 317.985 | 38.681 | 1.767 | 0.823 | -3.71 | -5.559 |
| Almeida et al. | 2025 | 318.093 | 38.586 | – | – | – | – |
| Alfonso et al. | 2024 | 318.031 | 38.782 | 1.741 | 0.831 | -3.706 | – |
| Zhang et al. | 2024 | 317.963 | 38.545 | – | – | – | – |
| 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 | – | – | – |
| Hunt & Reffert | 2023 | 317.963 | 38.545 | 1.771 | 0.828 | -3.686 | -6.493 |
| Just et al. | 2023 | 318.002 | 38.607 | – | – | – | – |
| He et al. | 2022 | 317.955 | 38.656 | 1.767 | 0.809 | -3.724 | – |
| Tarricq et al. | 2022 | 317.926 | 38.543 | 1.768 | 0.826 | -3.708 | – |
| 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 | – |
| Liu & Pang | 2019 | 318.043 | 38.763 | 1.774 | 0.78 | -3.652 | – |
| Bossini et al. | 2019 | 317.933 | 38.638 | – | – | – | – |
| Soubiran et al. | 2018 | 317.933 | 38.638 | – | – | – | -4.44 |
| Bica et al. | 2019 | 317.992 | 38.599 | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 317.933 | 38.638 | 1.762 | 0.8 | -3.679 | – |
| Kharchenko et al. | 2016 | 318.002 | 38.607 | – | – | – | – |
| Kharchenko et al. | 2013 | 318.007 | 38.61 | – | 0.4 | -4.95 | – |
| Piskunov et al. | 2008 | 317.993 | 38.599 | – | – | – | – |
| Kharchenko et al. | 2005 | 318.0 | 38.6 | – | 1.04 | -4.22 | – |
| Dias et al. | 2002 | 318.0 | 38.6 | – | 1.04 | -4.22 | – |
💡 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 0.56 | 0.28 | – | 285 | – | 156 | – | – |
| Alfonso et al. | 2024 | 0.56 | 0.13 | – | 432 | -0.051 | – | – | – |
| Zhang et al. | 2024 | – | – | – | – | -0.073* | – | – | – |
| Hunt & Reffert | 2024 | – | – | – | – | – | 609* | – | – |
| Cavallo et al. | 2024 | 0.56 | 0.36 | – | 132 | 0.250 | – | – | – |
| Hunt & Reffert | 2023 | 0.54 | 0.11 | 0.48 | 184 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 85 | – | 29 | – | – |
| He et al. | 2022 | – | 0.35 | – | 71 | – | – | – | – |
| Tarricq et al. | 2022 | 0.56 | – | – | 302 | – | – | – | – |
| Dias et al. | 2021 | 0.56 | 0.28 | – | 285 | -0.052 | – | – | – |
| Cantat-Gaudin et al. | 2020 | 0.56 | 0.13 | – | 288 | – | – | – | – |
| Liu & Pang | 2019 | – | – | – | 65 | -0.250 | – | – | – |
| Bossini et al. | 2019 | 0.53 | 0.09 | – | 426 | 0.000 | – | – | – |
| Soubiran et al. | 2018 | 0.56 | – | – | – | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 0.56 | – | – | – | – | – | – | – |
| Kharchenko et al. | 2016 | 0.50 | 0.00 | – | 85 | – | – | – | – |
| Kharchenko et al. | 2013 | 0.50 | 0.00 | – | 85 | – | – | – | – |
| Piskunov et al. | 2008 | 0.45 | 0.00 | – | 138 | – | – | – | – |
| Kharchenko et al. | 2005 | 0.45 | 0.00 | – | 138 | – | – | – | – |
| Dias et al. | 2002 | 0.45 | 0.00 | – | 138 | – | – | – | – |
💡 Note: The parameters are sometimes
transformed from their original values to match the format of the
columns shown here, see FAQ.
The columns DAv, Bfr, BSS correspond to differential
extinction, binary fraction, and blue stragglers, respectively.
BSS values can be listed as fractions or integers.
(*): indicates that this parameter is
assigned more than one value in the corresponding reference.
