Roslund 1
(MWSC 3169; OCL 112)
0.71
UTI
0.41
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
9.1 [arcmin]
- CN 0.41 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Roslund 1 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
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 | 296.243 | 17.523 | 1.134 | -0.861 | -5.832 | -4.783 |
| Hunt & Reffert | 2024 | 296.264 | 17.549 | 1.126 | -0.874 | -5.828 | -5.623 |
| Cavallo et al. | 2024 | 296.247 | 17.491 | 1.129 | â | â | â |
| Hunt & Reffert | 2023 | 296.264 | 17.549 | 1.126 | -0.874 | -5.828 | -5.623 |
| Just et al. | 2023 | 296.273 | 17.508 | â | â | â | â |
| Bica et al. | 2019 | 296.288 | 17.519 | â | â | â | â |
| Kharchenko et al. | 2016 | 296.273 | 17.508 | â | â | â | â |
| Dias et al. | 2014 | 296.25 | 17.517 | â | -2.91 | 0.28 | â |
| Kharchenko et al. | 2013 | 296.28 | 17.51 | â | 0.4 | -7.21 | â |
| Piskunov et al. | 2008 | 296.241 | 17.522 | â | â | â | â |
| Kharchenko et al. | 2005 | 296.25 | 17.52 | â | 1.18 | -7.08 | â |
| Kharchenko et al. | 2003 | 296.28 | 17.53 | â | 0.01 | -4.63 | â |
| Dias et al. | 2002 | 296.25 | 17.517 | â | 1.18 | -7.08 | 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 | 115* | â | â |
| Cavallo et al. | 2024 | 0.86 | 1.15 | â | 105 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.85 | 0.99 | 0.81 | 169 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 582 | â | 13 | â | â |
| Kharchenko et al. | 2016 | 0.79 | 0.16 | â | 582 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.79 | 0.16 | â | 582 | â | â | â | â |
| Piskunov et al. | 2008 | 0.67 | 0.16 | â | 295 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.67 | 0.16 | â | 295 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.83 | 0.46 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.67 | 0.16 | â | 295 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.