Loden 402
(MWSC 1954)
0.18
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.39
Clit
1.0
Cdup
Core radius and density
8.0 [pc], 0.05 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.39 Poorly studied
- Cdup 1.0 Unique
Overview
Loden 402 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.27 kpc) differs significantly from the median photometric distance (~1.98 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 | 173.189 | -60.682 | 0.19 | -6.286 | 1.719 | -11.389 |
| Just et al. | 2023 | 173.077 | -60.702 | â | â | â | â |
| Bica et al. | 2019 | 173.161 | -60.711 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -7.5 | 1.62 | â |
| Dib et al. | 2018 | 173.085 | -60.705 | â | â | â | â |
| Sampedro et al. | 2017 | 173.217 | -60.717 | â | -3.06 | -3.79 | â |
| Joshi et al. | 2016 | 173.085 | -60.705 | â | â | â | â |
| Kharchenko et al. | 2016 | 173.077 | -60.702 | â | â | â | â |
| Dias et al. | 2014 | 173.217 | -60.717 | â | -3.23 | -3.59 | â |
| Kharchenko et al. | 2013 | 173.085 | -60.705 | â | -7.4 | 0.9 | -3.0 |
| Gozha et al. | 2012 | 173.217 | -60.717 | â | â | â | â |
| Piskunov et al. | 2008 | 173.161 | -60.711 | â | â | â | â |
| Kharchenko et al. | 2007 | 173.22 | -60.72 | â | 0.15 | â | -3.0 |
| Kharchenko et al. | 2005 | 173.17 | -60.72 | â | -6.9 | -0.53 | â |
| Dias et al. | 2002 | 173.217 | -60.717 | â | -3.23 | -3.59 | -3.0 |
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 | 1.98 | 0.775 | â | 251 | â | 3311 | â | â |
| Just et al. | 2023 | â | â | â | 251 | â | 268 | â | â |
| Dib et al. | 2018 | 1.51 | â | â | 251 | â | â | â | â |
| Joshi et al. | 2016 | 1.51 | 0.98 | â | 251 | â | 3311 | â | â |
| Kharchenko et al. | 2016 | 1.51 | 0.98 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.51 | 0.98 | â | 251 | â | â | â | â |
| Gozha et al. | 2012 | 2.45 | â | â | 158 | â | 3311 | â | â |
| Piskunov et al. | 2008 | 2.45 | 0.57 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.45 | 0.57 | â | 158 | â | â | â | â |
| Dias et al. | 2002 | 2.45 | 0.57 | â | 158 | â | â | â | â |
MOCA
