Loden 615
(MWSC 2015; OCL 879.1; ESO 095 06)
0.18
UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.39
Clit
1.0
Cdup
Core radius and density
3.5 [pc], 0.08 [pc-2]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.12 Very low quality
- Clit 0.39 Poorly studied
- Cdup 1.0 Unique
Overview
Loden 615 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below 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 (~4.13 kpc) differs significantly from the median photometric distance (~0.92 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 | 185.2 | -64.808 | 0.242 | -7.482 | 0.464 | -13.554 |
| Just et al. | 2023 | 185.16 | -64.772 | â | â | â | â |
| Bica et al. | 2019 | 185.165 | -64.786 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -7.7 | -0.64 | â |
| Dib et al. | 2018 | 185.17 | -64.775 | â | â | â | â |
| Sampedro et al. | 2017 | 185.162 | -64.783 | â | -3.56 | -0.99 | â |
| Joshi et al. | 2016 | 185.17 | -64.775 | â | â | â | â |
| Kharchenko et al. | 2016 | 185.16 | -64.772 | â | â | â | â |
| Dias et al. | 2014 | 185.163 | -64.783 | â | -5.31 | -0.28 | â |
| Kharchenko et al. | 2013 | 185.17 | -64.775 | â | -8.69 | -2.48 | â |
| Piskunov et al. | 2008 | 185.145 | -64.775 | â | â | â | â |
| Kharchenko et al. | 2005 | 185.16 | -64.78 | â | -6.97 | -2.24 | â |
| Kharchenko et al. | 2003 | 185.16 | -64.77 | â | -6.8 | -2.67 | â |
| Dias et al. | 2002 | 185.162 | -64.783 | â | -6.8 | -2.67 | â |
| Lynga | 1987 | 185.168 | -64.776 | 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 | 0.915 | 0.16 | â | 427 | â | 98 | â | â |
| Just et al. | 2023 | â | â | â | 427 | â | 72 | â | â |
| Dib et al. | 2018 | 0.83 | â | â | 427 | â | â | â | â |
| Joshi et al. | 2016 | 0.83 | 0.16 | â | 427 | â | 123 | â | â |
| Kharchenko et al. | 2016 | 0.83 | 0.16 | â | 427 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.83 | 0.16 | â | 427 | â | â | â | â |
| Piskunov et al. | 2008 | 1.00 | 0.16 | â | 427 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 0.16 | â | 427 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.67 | 0.63 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.16 | â | 427 | â | â | â | â |
MOCA
