Ruprecht 77
(VDBH 68; MWSC 1670; OCL 784; vdBergh-Hagen 68; ESO 166 12)
0.74
UTI
0.52
CN
1.0
Cdens
0.5
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 77 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Metal-rich
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 141.801 | -55.108 | 0.274 | -6.255 | 4.806 | 41.115 |
| Hunt & Reffert | 2024 | 141.842 | -55.098 | 0.278 | -6.234 | 4.83 | 41.115 |
| Celli et al. | 2024 | 141.784 | -55.126 | â | â | â | â |
| Cavallo et al. | 2024 | 141.807 | -55.104 | 0.28 | â | â | â |
| Hunt & Reffert | 2023 | 141.842 | -55.098 | 0.278 | -6.234 | 4.83 | 41.115 |
| Just et al. | 2023 | 141.79 | -55.12 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 141.821 | -55.119 | 0.242 | -6.286 | 4.84 | â |
| Cantat-Gaudin & Anders | 2020 | 141.821 | -55.119 | 0.242 | -6.286 | 4.84 | â |
| Bica et al. | 2019 | 141.758 | -55.116 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 141.821 | -55.119 | 0.242 | -6.286 | 4.84 | â |
| Loktin & Popova | 2017 | 141.765 | -55.123 | â | -10.819 | 0.743 | â |
| Kharchenko et al. | 2016 | 141.79 | -55.12 | â | â | â | â |
| Dias et al. | 2014 | 141.767 | -55.117 | â | 1.12 | -0.89 | â |
| Kharchenko et al. | 2013 | 141.795 | -55.123 | â | -4.36 | 2.48 | â |
| van den Bergh | 2006 | 141.775 | -55.117 | â | â | â | â |
| Dias et al. | 2002 | 141.767 | -55.117 | â | 1.12 | -0.89 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 426* | â | â |
| Celli et al. | 2024 | â | â | â | 12 | â | 192 | â | â |
| Cavallo et al. | 2024 | 4.04 | 1.93 | â | 68 | 0.800 | â | â | â |
| Hunt & Reffert | 2023 | 3.17 | 1.55 | 1.77 | 202 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 89 | â | 971 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.11 | 1.92 | â | 12 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.69 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.69 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 4.14 | 1.92 | â | 33 | â | â | â | â |
| Kharchenko et al. | 2016 | 4.09 | 2.13 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.09 | 2.13 | â | 89 | â | â | â | â |
| van den Bergh | 2006 | 4.13 | 1.92 | â | 32 | â | â | â | â |
| Dias et al. | 2002 | 4.13 | 1.93 | â | 32 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.