Roslund 4
0.85
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
3.6 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Roslund 4 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 301.189 | 29.202 | 0.423 | -2.174 | -5.11 | -4.256 |
| Hunt & Reffert | 2024 | 301.214 | 29.191 | 0.433 | -2.231 | -5.17 | 55.191 |
| Celli et al. | 2024 | 301.199 | 29.196 | â | â | â | â |
| Cavallo et al. | 2024 | 301.105 | 29.1 | 0.434 | â | â | â |
| Hunt & Reffert | 2023 | 301.214 | 29.191 | 0.433 | -2.231 | -5.17 | 55.191 |
| Jaehnig et al. | 2021 | 301.212 | 29.188 | 0.46 | -2.168 | -5.089 | â |
| Rain et al. | 2021 | 301.199 | 29.196 | 0.423 | -2.166 | -5.057 | â |
| Cantat-Gaudin et al. | 2020 | 301.199 | 29.196 | 0.423 | -2.166 | -5.057 | â |
| Cantat-Gaudin & Anders | 2020 | 301.199 | 29.196 | 0.423 | -2.166 | -5.057 | â |
| Cantat-Gaudin et al. | 2018 | 301.199 | 29.196 | 0.423 | -2.166 | -5.057 | â |
| Loktin & Popova | 2017 | 301.23 | 29.217 | â | -5.016 | -5.668 | -15.7 |
| Dias et al. | 2014 | 301.225 | 29.217 | â | -2.9 | -4.91 | â |
| Gozha et al. | 2012 | 301.225 | 29.217 | â | â | â | â |
| Kharchenko et al. | 2007 | 301.23 | 29.22 | â | 0.04 | â | â |
| van den Bergh | 2006 | 301.225 | 29.217 | â | â | â | â |
| Dias et al. | 2002 | 301.225 | 29.217 | â | -2.9 | -4.91 | -15.7 |
| Dambis | 1999 | 301.225 | 29.217 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 918* | â | â |
| Celli et al. | 2024 | â | â | â | 17 | â | 315 | â | â |
| Cavallo et al. | 2024 | 2.18 | 3.23 | â | 10 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 2.15 | 3.30 | 2.73 | 10 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.17* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.21 | 2.82 | â | 4 | â | â | â | 0 |
| Cantat-Gaudin et al. | 2020 | 2.06 | 2.33 | â | 17 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.21 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.21 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.51 | 2.99 | â | 34 | â | â | â | â |
| Gozha et al. | 2012 | 2.00 | â | â | 4 | â | â | â | â |
| van den Bergh | 2006 | 2.51 | 3.07 | â | 28 | â | â | â | â |
| Dias et al. | 2002 | 2.00 | 2.82 | â | 4 | â | â | â | â |
| Dambis | 1999 | 2.19 | 2.83 | â | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.