ASCC 21
(OCSN 129)
0.95
UTI
0.77
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
19.3 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
ASCC 21 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below 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 absorption parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a small 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 | 82.229 | 3.545 | 2.893 | 1.456 | -0.613 | 15.495 |
| Liu et al. | 2025 | 82.21 | 3.61 | 2.9 | 1.53 | -0.58 | 10.17 |
| Li et al. | 2025 | 82.179 | 3.527 | 2.866 | 1.404 | -0.632 | â |
| Almeida et al. | 2025 | 82.142 | 3.477 | â | â | â | â |
| Alfonso et al. | 2024 | 81.835 | 2.466 | 2.844 | 1.436 | -0.307 | â |
| Zhang et al. | 2024 | 82.212 | 3.607 | â | â | â | â |
| Hunt & Reffert | 2024 | 82.212 | 3.607 | 2.902 | 1.532 | -0.576 | 10.168 |
| Celli et al. | 2024 | 82.179 | 3.527 | â | â | â | â |
| Cavallo et al. | 2024 | 82.364 | 3.309 | 2.902 | â | â | â |
| Hunt & Reffert | 2023 | 82.212 | 3.607 | 2.902 | 1.532 | -0.576 | 10.168 |
| Almeida et al. | 2023 | 82.171 | 3.439 | â | â | â | â |
| Qin et al. | 2023 | 82.15 | 3.58 | 2.91 | 1.48 | -0.6 | 16.95 |
| Dias et al. | 2021 | 82.142 | 3.477 | 2.893 | 1.381 | -0.61 | 15.313 |
| Cantat-Gaudin et al. | 2020 | 82.179 | 3.527 | 2.866 | 1.404 | -0.632 | â |
| Donor et al. | 2020 | 82.26 | 3.56 | â | 1.28 | -0.29 | 20.0 |
| Zhong et al. | 2020 | 82.179 | 3.527 | â | 1.404 | -0.632 | 28.751 |
| Cantat-Gaudin & Anders | 2020 | 82.179 | 3.527 | 2.866 | 1.404 | -0.632 | â |
| Dias et al. | 2019 | 82.179 | 3.527 | 2.866 | 1.404 | -0.632 | 16.034 |
| Bossini et al. | 2019 | 82.179 | 3.527 | â | â | â | â |
| Soubiran et al. | 2018 | 82.179 | 3.527 | â | â | â | 18.7 |
| Cantat-Gaudin et al. | 2018 | 82.179 | 3.527 | 2.866 | 1.404 | -0.632 | â |
| Dias et al. | 2014 | 82.246 | 3.65 | â | 1.6 | -3.82 | â |
| Gozha et al. | 2012 | 82.246 | 3.65 | â | â | â | â |
| Piskunov et al. | 2008 | 82.236 | 3.646 | â | â | â | â |
| Kharchenko et al. | 2007 | 82.24 | 3.65 | â | 0.8 | â | 19.77 |
| Piskunov et al. | 2007 | 82.236 | 3.646 | â | â | â | â |
| Kharchenko et al. | 2005 | 82.24 | 3.65 | â | 0.52 | -0.62 | 19.9 |
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 | 0.34 | 0.13 | 0.7 | 12 | -0.034 | 367 | 0.27 | â |
| Liu et al. | 2025 | 0.32 | 0.02 | â | 16 | â | â | â | â |
| Li et al. | 2025 | 0.31 | 0.17 | â | 11 | -0.142 | â | â | â |
| Almeida et al. | 2025 | 0.34 | 0.24 | â | 13 | â | 106 | â | â |
| Alfonso et al. | 2024 | 0.34 | 0.10 | â | 10 | -0.008 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.059(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 63(1) | â | â |
| Celli et al. | 2024 | â | â | â | 9 | â | 46 | â | â |
| Cavallo et al. | 2024 | 0.34 | 0.59 | â | 7 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.33 | 0.14 | 0.70 | 7 | â | â | â | â |
| Almeida et al. | 2023 | 0.34 | 0.28 | â | 10 | -0.118 | 367(1) | 0.27 | â |
| Qin et al. | 2023 | 0.39 | 0.34 | â | 9 | â | â | â | â |
| Dias et al. | 2021 | 0.34 | 0.24 | â | 13 | -0.008 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.34 | 0.10 | â | 9 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.180 | â | â | â |
| Zhong et al. | 2020 | 0.31 | 0.12 | â | 7032 | -0.108 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.35 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 0.35 | 0.16 | â | 12 | 0.169 | â | â | â |
| Bossini et al. | 2019 | 0.31 | 0.12 | â | 11 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.35 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.35 | â | â | â | â | â | â | â |
| Gozha et al. | 2012 | 0.50 | â | â | 13 | â | 851 | â | â |
| Piskunov et al. | 2008 | 0.50 | 0.09 | â | 13 | â | 1102(1) | â | â |
| Piskunov et al. | 2007 | 0.50 | 0.09 | â | 13 | â | 557 | â | â |
| Kharchenko et al. | 2005 | 0.50 | 0.09 | â | 13 | 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 7 along with Briceno_1, and of multiple system 5 along with ASCC_20 and Briceno_1.
Palma et al. (2025)
Classified as genetic pair P184, along with Briceno_1.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.