ASCC 59
(MWSC 1793)
0.16
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
19
Core radius and density
3.1 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
ASCC 59 is a sparse, very loose object of very 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 (~2.04 kpc) differs significantly from the median photometric distance (~0.53 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 155.31 | -57.72 | 0.49 | -8.812 | 4.829 | 2.596 |
| Hunt & Reffert | 2023 | 155.396 | -57.679 | 0.501 | -8.778 | 4.822 | â |
| Bica et al. | 2019 | 155.051 | -57.646 | â | â | â | â |
| Dib et al. | 2018 | 155.115 | -57.675 | â | â | â | â |
| Sampedro et al. | 2017 | 155.054 | -57.65 | â | -3.65 | 1.45 | â |
| Joshi et al. | 2016 | 155.115 | -57.675 | â | â | â | â |
| Kharchenko et al. | 2016 | 155.109 | -57.672 | â | â | â | â |
| Dias et al. | 2014 | 155.054 | -57.65 | â | -3.64 | 1.54 | â |
| Kharchenko et al. | 2013 | 155.115 | -57.675 | â | -4.84 | 3.18 | â |
| Piskunov et al. | 2008 | 155.051 | -57.646 | â | â | â | â |
| Kharchenko et al. | 2005 | 155.05 | -57.65 | â | -4.99 | 3.65 | â |
| Dias et al. | 2002 | 155.054 | -57.65 | â | -4.99 | 3.65 | 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 | 0.53 | 0.16 | 0.41 | 343 | â | 155 | â | â |
| Hunt & Reffert | 2023 | 1.88 | 0.34 | 0.41 | 4539 | â | â | â | â |
| Dib et al. | 2018 | 0.51 | â | â | 288 | â | â | â | â |
| Joshi et al. | 2016 | 0.51 | 0.16 | â | 288 | â | 155 | â | â |
| Kharchenko et al. | 2016 | 0.51 | 0.16 | â | 288 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.51 | 0.16 | â | 288 | â | â | â | â |
| Piskunov et al. | 2008 | 0.55 | 0.16 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.55 | 0.16 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 0.55 | 0.16 | â | 398 | â | â | â | â |
MOCA


Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.88 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.88 (50th percentile).