Ruprecht 92
(MWSC 1866; OCL 834; ESO 128 17)
0.37
UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
6.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.25 Low quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 92 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 a massive, near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~6.06 kpc) differs significantly from the median photometric distance (~2.36 kpc).
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 163.465 | -61.77 | 0.165 | -6.744 | 2.906 | 23.649 |
| He et al. | 2023 | 163.452 | -61.747 | 0.184 | -6.016 | 2.214 | â |
| Just et al. | 2023 | 163.374 | -61.697 | â | â | â | â |
| Bica et al. | 2019 | 163.451 | -61.74 | â | â | â | â |
| Loktin & Popova | 2017 | 163.44 | -61.75 | â | -4.346 | -3.437 | -15.3 |
| Kharchenko et al. | 2016 | 163.374 | -61.697 | â | â | â | â |
| Dias et al. | 2014 | 163.446 | -61.75 | â | -2.44 | -2.06 | â |
| Kharchenko et al. | 2013 | 163.38 | -61.7 | â | -3.22 | 2.78 | -15.3 |
| Gozha et al. | 2012 | 163.446 | -61.75 | â | â | â | â |
| Piskunov et al. | 2008 | 163.28 | -61.701 | â | â | â | â |
| Kharchenko et al. | 2007 | 163.44 | -61.75 | â | 0.18 | â | -15.6 |
| van den Bergh | 2006 | 163.3 | -61.717 | â | â | â | â |
| Kharchenko et al. | 2005 | 163.29 | -61.71 | â | -2.05 | 0.5 | â |
| Kharchenko et al. | 2003 | 163.36 | -61.69 | â | -5.32 | 1.22 | â |
| Dias et al. | 2002 | 163.446 | -61.75 | â | -2.44 | -2.06 | -15.6 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| He et al. | 2023 | 4.68 | 1.15 | â | 40 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 45 | â | 632 | â | â |
| Loktin & Popova | 2017 | 2.44 | 1.34 | â | 74 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.21 | 1.23 | â | 45 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.21 | 1.23 | â | 45 | 0.201 | â | â | â |
| Gozha et al. | 2012 | 2.36 | â | â | 63 | â | 3236 | â | â |
| Piskunov et al. | 2008 | 2.36 | 1.43 | â | 34 | â | â | â | â |
| van den Bergh | 2006 | 2.36 | 1.43 | â | 63 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.36 | 1.43 | â | 34 | â | â | â | â |
| Kharchenko et al. | 2003 | 2.38 | 0.93 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.21 | 1.23 | â | 45 | 0.201 | â | â | â |
