IRAS 02130+5509
0.24
UTI
0.0
CN
0.31
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
7.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.31 Loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
IRAS 02130+5509 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
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.
Relatively 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 | 34.173 | 55.353 | 0.563 | -0.737 | -0.876 | -56.918 |
| Zhang et al. | 2024 | 34.137 | 55.412 | â | â | â | â |
| Hunt & Reffert | 2024 | 34.137 | 55.412 | 0.567 | -0.734 | -0.889 | â |
| Cavallo et al. | 2024 | 34.237 | 55.261 | 0.561 | â | â | â |
| Hunt & Reffert | 2023 | 34.137 | 55.412 | 0.567 | -0.734 | -0.889 | 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 | -0.173* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 96* | â | â |
| Cavallo et al. | 2024 | 1.65 | 0.75 | â | 25 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 1.73 | 0.80 | 0.96 | 33 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.