Loden 1225
(MWSC 2204; OCL 915.5; ESO 133 12)
0.28
UTI
0.0
CN
0.01
Cdens
0.62
CC3
0.39
Clit
1.0
Cdup
Core radius and density
5.0 [pc], 0.05 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.39 Poorly studied
- Cdup 1.0 Unique
Overview
Loden 1225 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~7.54 kpc) differs significantly from the median photometric distance (~1.38 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 | 212.205 | -59.761 | 0.133 | -6.997 | -2.067 | -41.635 |
| Just et al. | 2023 | 212.328 | -59.722 | â | â | â | â |
| Bica et al. | 2019 | 212.245 | -59.723 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -5.51 | -2.83 | â |
| Dib et al. | 2018 | 212.34 | -59.725 | â | â | â | â |
| Sampedro et al. | 2017 | 212.262 | -59.717 | â | -3.24 | -3.76 | â |
| Joshi et al. | 2016 | 212.34 | -59.725 | â | â | â | â |
| Kharchenko et al. | 2016 | 212.328 | -59.722 | â | â | â | â |
| Dias et al. | 2014 | 212.262 | -59.717 | â | -2.61 | -3.35 | â |
| Kharchenko et al. | 2013 | 212.34 | -59.725 | â | -9.95 | 0.25 | â |
| Piskunov et al. | 2008 | 212.264 | -59.72 | â | â | â | â |
| Kharchenko et al. | 2005 | 212.26 | -59.72 | â | -9.99 | 0.25 | â |
| Kharchenko et al. | 2003 | 212.23 | -59.72 | â | -9.83 | -0.76 | â |
| Dias et al. | 2002 | 212.262 | -59.717 | â | -2.61 | -3.35 | â |
| Lynga | 1987 | 212.289 | -59.726 | â | â | â | 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 | 1.38 | 0.63 | â | 468 | â | 456 | â | â |
| Just et al. | 2023 | â | â | â | 468 | â | 296 | â | â |
| Dib et al. | 2018 | 1.33 | â | â | 468 | â | â | â | â |
| Joshi et al. | 2016 | 1.33 | 0.79 | â | 468 | â | 617 | â | â |
| Kharchenko et al. | 2016 | 1.33 | 0.79 | â | 468 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.33 | 0.79 | â | 468 | â | â | â | â |
| Piskunov et al. | 2008 | 1.50 | 0.63 | â | 468 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.50 | 0.63 | â | 468 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.43 | 0.32 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 0.63 | â | 468 | â | â | â | â |
MOCA
