ASCC 18
(MWSC 541)
0.84
UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
31.5 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 18 is a moderately populated, 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 (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with 2 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 | 81.526 | 0.321 | 2.4 | 0.153 | 1.392 | 25.207 |
| Zhang et al. | 2024 | 81.33 | 0.368 | â | â | â | â |
| Cavallo et al. | 2024 | 81.322 | 0.317 | 2.415 | â | â | â |
| Hunt & Reffert | 2023 | 81.33 | 0.368 | 2.415 | 0.156 | 1.373 | 26.158 |
| Just et al. | 2023 | 81.555 | 0.901 | â | â | â | â |
| Donor et al. | 2020 | 81.562 | 0.9 | â | 1.13 | -0.31 | 21.2 |
| Bica et al. | 2019 | 81.54 | 0.824 | â | â | â | â |
| Kharchenko et al. | 2016 | 81.555 | 0.901 | â | â | â | â |
| Dias et al. | 2014 | 81.542 | 0.82 | â | 2.67 | -1.96 | â |
| Kharchenko et al. | 2013 | 81.562 | 0.9 | â | 3.21 | -0.96 | 24.4 |
| Gozha et al. | 2012 | 81.542 | 0.82 | â | â | â | â |
| Piskunov et al. | 2008 | 81.532 | 0.819 | â | â | â | â |
| Kharchenko et al. | 2007 | 81.54 | 0.82 | â | 0.62 | â | 24.4 |
| Kharchenko et al. | 2005 | 81.54 | 0.82 | â | 0.89 | -0.02 | 13.39 |
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 | 0.4 | 0.19 | 0.76 | 13 | 0.063 | 262 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.063(1) | â | â | â |
| Cavallo et al. | 2024 | 0.40 | 0.40 | â | 6 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 0.40 | 0.23 | 0.76 | 9 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 14 | â | 10 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.140 | â | â | â |
| Kharchenko et al. | 2016 | 0.31 | 0.19 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.31 | 0.19 | â | 14 | â | â | â | â |
| Gozha et al. | 2012 | 0.50 | â | â | 13 | â | 513 | â | â |
| Piskunov et al. | 2008 | 0.50 | 0.19 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.50 | 0.19 | â | 13 | â | â | â | â |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.