Alicante 1
(MWSC 323)
0.59
UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
12.3 [N/pc2]
- CN 0.31 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
Alicante 1 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. 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 | 99999β | 59.799 | 57.234 | 0.256 | -0.069 | 0.392 | β |
| Just et al. | 2023 | 59.772 | 57.239 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 59.825 | 57.237 | β | -0.183 | 0.607 | β |
| Loktin & Popova | 2017 | 59.82 | 57.237 | β | -1.926 | 0.4 | -32.4 |
| Kharchenko et al. | 2016 | 59.772 | 57.239 | β | β | β | β |
| Dias et al. | 2014 | 59.825 | 57.237 | β | -1.51 | 1.6 | β |
| Kharchenko et al. | 2013 | 59.785 | 57.24 | β | -1.76 | 1.36 | -32.4 |
| Kharchenko et al. | 2012 | 59.785 | 57.24 | β | -1.76 | 1.36 | -32.4 |
| Dias et al. | 2002 | 59.825 | 57.237 | β | -1.76 | 1.36 | -32.4 |
π‘ 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 | 99999β | 4.3 | 1.86 | β | 2 | β | 63 | β | β |
| Just et al. | 2023 | β | β | β | 2 | β | 63 | β | β |
| Loktin & Popova | 2017 | 2.27 | 1.27 | β | 12 | β | β | β | β |
| Kharchenko et al. | 2016 | 4.30 | 1.86 | β | 2 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.30 | 1.86 | β | 2 | β | β | β | β |
| Kharchenko et al. | 2012 | 4.30 | 1.86 | β | 2 | β | β | β | β |
| Dias et al. | 2002 | 3.98 | 2.08 | β | 4 | β | β | β | β |
MOCA
