ASCC 54
(MWSC 1709)
0.24
UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.25 Low quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
ASCC 54 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.64 kpc) differs significantly from the median photometric distance (~1.20 kpc).
Note: This object shares a small 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 | 146.191 | -54.427 | 0.275 | -4.864 | 3.415 | 9.809 |
| Just et al. | 2023 | 146.192 | -54.431 | â | â | â | â |
| Bica et al. | 2019 | 146.229 | -54.44 | â | â | â | â |
| Kharchenko et al. | 2016 | 146.192 | -54.431 | â | â | â | â |
| Dias et al. | 2014 | 146.192 | -54.44 | â | -3.73 | 0.14 | â |
| Kharchenko et al. | 2013 | 146.197 | -54.435 | â | -8.17 | 1.75 | â |
| Piskunov et al. | 2008 | 146.191 | -54.435 | â | â | â | â |
| Kharchenko et al. | 2005 | 146.19 | -54.44 | â | -7.73 | 1.08 | â |
| Dias et al. | 2002 | 146.192 | -54.44 | â | -7.73 | 1.08 | 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 | 1.2 | 0.16 | â | 712 | â | 284 | â | â |
| Just et al. | 2023 | â | â | â | 733 | â | 284 | â | â |
| Kharchenko et al. | 2016 | 1.75 | 0.32 | â | 733 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.75 | 0.32 | â | 733 | â | â | â | â |
| Piskunov et al. | 2008 | 1.20 | 0.16 | â | 692 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.20 | 0.16 | â | 692 | â | â | â | â |
| Dias et al. | 2002 | 1.20 | 0.16 | â | 692 | â | â | â | â |
MOCA
