Roslund 7
(MWSC 3416; OCL 187)
0.84
UTI
0.75
CN
0.69
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
15.0 [arcmin]
- CN 0.75 Rich
- Cdens 0.69 Moderately dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Roslund 7 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 313.196 | 37.891 | 0.781 | 1.734 | -0.395 | -14.414 |
| Li et al. | 2025 | 313.196 | 37.847 | 0.78 | 1.729 | -0.36 | â |
| Almeida et al. | 2025 | 313.224 | 37.829 | â | â | â | â |
| Zhang et al. | 2024 | 313.213 | 37.92 | â | â | â | â |
| Hunt & Reffert | 2024 | 313.213 | 37.92 | 0.776 | 1.707 | -0.406 | -16.19 |
| Cavallo et al. | 2024 | 313.224 | 37.835 | 0.777 | â | â | â |
| Hunt & Reffert | 2023 | 313.213 | 37.92 | 0.776 | 1.707 | -0.406 | -16.19 |
| Almeida et al. | 2023 | 313.198 | 37.807 | â | â | â | â |
| Just et al. | 2023 | 313.089 | 37.897 | â | â | â | â |
| Tarricq et al. | 2022 | 313.126 | 37.939 | 0.777 | 1.749 | -0.404 | â |
| Dias et al. | 2021 | 313.224 | 37.829 | 0.778 | 1.719 | -0.354 | â |
| Cantat-Gaudin et al. | 2020 | 313.196 | 37.847 | 0.78 | 1.729 | -0.36 | â |
| Cantat-Gaudin & Anders | 2020 | 313.196 | 37.847 | 0.78 | 1.729 | -0.36 | â |
| Soubiran et al. | 2018 | 313.196 | 37.847 | â | â | â | -12.72 |
| Bica et al. | 2019 | 313.125 | 38.065 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 313.196 | 37.847 | 0.78 | 1.729 | -0.36 | â |
| Kharchenko et al. | 2016 | 313.089 | 37.897 | â | â | â | â |
| Dias et al. | 2014 | 313.033 | 37.896 | â | -3.55 | -5.75 | â |
| Kharchenko et al. | 2013 | 313.095 | 37.9 | â | -0.05 | -0.11 | -22.0 |
| Gozha et al. | 2012 | 313.033 | 37.896 | â | â | â | â |
| Piskunov et al. | 2008 | 313.092 | 37.892 | â | â | â | â |
| Kharchenko et al. | 2007 | 313.03 | 37.9 | â | 0.43 | â | -22.0 |
| Piskunov et al. | 2007 | 313.092 | 37.892 | â | â | â | â |
| Kharchenko et al. | 2005 | 313.09 | 37.9 | â | 1.2 | 0.42 | â |
| Kharchenko et al. | 2003 | 313.09 | 37.93 | â | 0.5 | -0.4 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.12 | 0.66 | â | 664 | -0.041 | â | â | â |
| Almeida et al. | 2025 | 1.19 | 0.86 | â | 321 | â | 442 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.186* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 411* | â | â |
| Cavallo et al. | 2024 | 1.31 | 0.89 | â | 275 | 0.480 | â | â | â |
| Hunt & Reffert | 2023 | 1.22 | 0.94 | 1.93 | 175 | â | â | â | â |
| Almeida et al. | 2023 | 1.22 | 1.13 | â | 108 | -0.009 | 617* | 0.58 | â |
| Just et al. | 2023 | â | â | â | 398 | â | 61 | â | â |
| Tarricq et al. | 2022 | 1.17 | â | â | 162 | â | â | â | â |
| Dias et al. | 2021 | 1.19 | 0.86 | â | 321 | 0.171 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.20 | 0.49 | â | 126 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.24 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.24 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.24 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 0.74 | 0.62 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.74 | 0.62 | â | 398 | â | â | â | â |
| Gozha et al. | 2012 | 0.57 | â | â | 468 | â | 324 | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.62 | â | 468 | â | 312* | â | â |
| Piskunov et al. | 2007 | 0.70 | 0.62 | â | 468 | â | 124 | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.62 | â | 468 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.57 | 0.46 | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.