Ruprecht 110
(MWSC 2199; OCL 912; ESO 097 10)
0.19
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.42
Clit
1.0
Cdup
Nm (P>50%)
12
Core radius and density
9.9 [pc], 0.03 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 110 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.18 kpc) differs significantly from the median photometric distance (~1.24 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 211.35 | -67.388 | 0.193 | -4.161 | -2.822 | -48.811 |
| Just et al. | 2023 | 211.396 | -67.472 | â | â | â | â |
| Bica et al. | 2019 | 211.435 | -67.355 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -5.84 | -2.35 | â |
| Dib et al. | 2018 | 211.41 | -67.475 | â | â | â | â |
| Sampedro et al. | 2017 | 211.358 | -67.467 | â | -3.69 | -5.12 | â |
| Joshi et al. | 2016 | 211.41 | -67.475 | â | â | â | â |
| Kharchenko et al. | 2016 | 211.396 | -67.472 | â | â | â | â |
| Dias et al. | 2014 | 211.358 | -67.467 | â | -3.62 | -5.02 | â |
| Kharchenko et al. | 2013 | 211.41 | -67.475 | â | -11.67 | -4.0 | -34.4 |
| Piskunov et al. | 2008 | 211.36 | -67.468 | â | â | â | â |
| Piskunov et al. | 2007 | 211.36 | -67.468 | â | â | â | â |
| Kharchenko et al. | 2005 | 211.36 | -67.47 | â | -12.35 | -4.21 | â |
| Kharchenko et al. | 2003 | 211.42 | -67.45 | â | -13.32 | -5.19 | â |
| Dias et al. | 2002 | 211.358 | -67.467 | â | -3.6 | -5.01 | -36.65 |
| Lynga | 1987 | 211.607 | -67.575 | 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 | 1.24 | 0.49 | â | 501 | -0.296 | 282 | â | â |
| Just et al. | 2023 | â | â | â | 501 | â | 115 | â | â |
| Dib et al. | 2018 | 1.24 | â | â | 501 | â | â | â | â |
| Joshi et al. | 2016 | 1.24 | 0.98 | â | 501 | â | 331 | â | â |
| Kharchenko et al. | 2016 | 1.24 | 0.98 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.24 | 0.98 | â | 501 | -0.234 | â | â | â |
| Piskunov et al. | 2008 | 1.30 | 0.00 | â | 550 | â | 885(1) | â | â |
| Piskunov et al. | 2007 | 1.30 | 0.00 | â | 550 | â | 232 | â | â |
| Kharchenko et al. | 2005 | 1.30 | 0.00 | â | 550 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.80 | 1.10 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.30 | 0.00 | â | 550 | -0.359 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
