Ruprecht 139
(MWSC 2776; OCL 20; ESO 521 10)
0.78
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.7
Clit
0.98
Cdup
Radius (P>50% members)
5.5 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 0.98 Unique
Overview
Ruprecht 139 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.15 kpc) differs significantly from the median photometric distance (~0.59 kpc).
Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
Close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 270.229 | -23.526 | 0.318 | -0.009 | -1.413 | 1.346 |
| Hunt & Reffert | 2024 | 270.236 | -23.545 | 0.291 | 0.011 | -1.416 | -31.414 |
| Cavallo et al. | 2024 | 270.24 | -23.528 | 0.291 | â | â | â |
| Hunt & Reffert | 2023 | 270.236 | -23.545 | 0.291 | 0.011 | -1.416 | -31.414 |
| Just et al. | 2023 | 270.239 | -23.536 | â | â | â | â |
| Bica et al. | 2019 | 270.242 | -23.535 | â | â | â | â |
| Kharchenko et al. | 2016 | 270.239 | -23.536 | â | â | â | â |
| Dias et al. | 2014 | 270.263 | -23.533 | â | -1.77 | -1.41 | â |
| Kharchenko et al. | 2013 | 270.247 | -23.535 | â | 0.46 | -3.87 | â |
| Piskunov et al. | 2008 | 270.248 | -23.526 | â | â | â | â |
| Kharchenko et al. | 2005 | 270.25 | -23.53 | â | -1.1 | -2.19 | â |
| Kharchenko et al. | 2003 | 270.25 | -23.52 | â | -0.48 | -1.77 | â |
| Dias et al. | 2002 | 270.262 | -23.533 | â | -1.77 | -1.41 | 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 | 1070* | â | â |
| Cavallo et al. | 2024 | 3.12 | 4.22 | â | 11 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 3.12 | 4.03 | 2.68 | 11 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1122 | â | 13 | â | â |
| Kharchenko et al. | 2016 | 0.59 | 0.32 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.59 | 0.32 | â | 1122 | â | â | â | â |
| Piskunov et al. | 2008 | 0.55 | 0.46 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.55 | 0.46 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.83 | 0.46 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.55 | 0.46 | â | 1122 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.