LISC 3534
(OCSN 208)
0.72
UTI
0.85
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
52.1 [arcmin]
- CN 0.85 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
LISC 3534 is a rich, 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, young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 12.195 | 50.247 | 2.179 | 7.373 | -3.082 | -5.551 |
| Zhang et al. | 2024 | 12.088 | 49.906 | â | â | â | â |
| Hunt & Reffert | 2024 | 12.088 | 49.906 | 2.189 | 7.368 | -3.082 | -5.828 |
| Cavallo et al. | 2024 | 12.608 | 50.213 | 2.186 | â | â | â |
| Hunt & Reffert | 2023 | 12.088 | 49.906 | 2.189 | 7.368 | -3.082 | -5.828 |
| Qin et al. | 2023 | 11.97 | 50.3 | 2.18 | 7.39 | -3.1 | -5.02 |
| Li et al. | 2022 | 11.941 | 50.253 | 2.18 | 7.408 | -3.078 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.093* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 275* | â | â |
| Cavallo et al. | 2024 | 0.47 | 0.50 | â | 68 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.44 | 0.14 | 0.83 | 149 | â | â | â | â |
| Qin et al. | 2023 | 0.55 | 0.43 | â | 79 | â | â | â | â |
| Li et al. | 2022 | 0.41 | 0.55 | â | â | -0.642 | â | 0.42 | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.