ESO 559 02
(MWSC 1170)
0.06
UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
ESO 559 02 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~6.04 kpc) differs significantly from the median photometric distance (~17.78 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.
Extremely distant
High extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 109.541 | -18.592 | 0.166 | -0.824 | 1.608 | â |
| He et al. | 2023 | 109.523 | -18.596 | 0.098 | -0.598 | 1.193 | â |
| Bica et al. | 2019 | 109.525 | -18.59 | â | â | â | â |
| Dias et al. | 2002 | 109.521 | -18.595 | â | -3.56 | 5.53 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| He et al. | 2023 | 17.78 | 3.70 | â | 20 | â | â | â | â |
