NGC 2430
(MWSC 1298)
0.19
UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad)
0.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.12 Very low quality
- Clit 0.4 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 2430 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.84 kpc) differs significantly from the median photometric distance (~0.71 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 | 114.9 | -16.412 | 0.261 | -2.496 | 2.273 | â |
| Just et al. | 2023 | 114.911 | -16.378 | â | â | â | â |
| Loktin & Popova | 2017 | 114.915 | -16.375 | â | -0.818 | 1.064 | 2.8 |
| Kharchenko et al. | 2016 | 114.911 | -16.378 | â | â | â | â |
| Dias et al. | 2014 | 114.921 | -16.297 | â | -2.35 | 1.35 | 34.14 |
| Kharchenko et al. | 2013 | 114.916 | -16.38 | â | -2.74 | 2.09 | 2.8 |
| Piskunov et al. | 2008 | 114.894 | -16.348 | â | â | â | â |
| Kharchenko et al. | 2005 | 114.9 | -16.35 | â | -4.07 | 1.28 | 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 | 0.71 | 0.52 | â | 264 | 0.130 | 9 | â | â |
| Just et al. | 2023 | â | â | â | 50 | â | 9 | â | â |
| Loktin & Popova | 2017 | 1.91 | 0.00 | â | 813 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.71 | 0.52 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.71 | 0.52 | â | 50 | 0.130 | â | â | â |
| Piskunov et al. | 2008 | 0.65 | 0.53 | â | 479 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.65 | 0.53 | â | 479 | â | â | â | â |
MOCA
