Ruprecht 15
(MWSC 1175)
0.20
UTI
0.0
CN
0.0
Cdens
0.38
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
7.4 [pc], 0.02 [pc-2]
- CN 0.0 Sparse
- Cdens 0.0 Very loose
- CC3 0.38 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 15 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.33 kpc) differs significantly from the median photometric distance (~2.89 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 | 109.923 | -19.586 | 0.158 | -0.692 | 1.665 | 96.739 |
| Just et al. | 2023 | 109.876 | -19.628 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -1.68 | 1.45 | â |
| Loktin & Popova | 2017 | 109.89 | -19.629 | â | 1.039 | 6.567 | â |
| Sampedro et al. | 2017 | 109.888 | -19.633 | â | 0.7 | 2.4 | â |
| Kharchenko et al. | 2016 | 109.876 | -19.628 | â | â | â | â |
| Tadross | 2014 | 109.888 | -19.633 | â | â | â | â |
| Dias et al. | 2014 | 109.888 | -19.633 | â | -0.94 | 1.72 | â |
| Kharchenko et al. | 2013 | 109.882 | -19.63 | â | -0.21 | 6.12 | â |
| Bukowiecki et al. | 2011 | 109.896 | -19.591 | â | â | â | â |
| Dias et al. | 2002 | 109.888 | -19.633 | â | -0.21 | 6.12 | â |
| Lynga | 1987 | 109.922 | -19.646 | 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 | 2.89 | 1.24 | â | 562 | â | 188 | â | â |
| Just et al. | 2023 | â | â | â | 562 | â | 289 | â | â |
| Loktin & Popova | 2017 | 3.43 | 0.85 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.36 | 1.31 | â | 562 | â | â | â | â |
| Tadross | 2014 | 1.84 | 2.05 | â | 500 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.36 | 1.31 | â | 562 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 86 | â | â |
| Bukowiecki et al. | 2011 | 3.43(1) | 1.14 | â | 501 | â | â | â | â |
| Dias et al. | 2002 | 3.42 | 1.17 | â | 501 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
