FSR 0258
(MWSC 3408)
0.70
UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Stellar density (N50/rad)
33.9 [N/pc2]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0258 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.50 kpc) differs significantly from the median photometric distance (~1.24 kpc).
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 311.207 | 43.897 | 0.4 | -3.312 | -3.952 | -10.89 |
| Hunt & Reffert | 2024 | 311.206 | 43.895 | 0.404 | -3.292 | -3.948 | -67.208 |
| Cavallo et al. | 2024 | 311.216 | 43.9 | 0.391 | β | β | β |
| Hunt & Reffert | 2023 | 311.206 | 43.895 | 0.404 | -3.292 | -3.948 | -67.208 |
| Just et al. | 2023 | 311.192 | 43.885 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 311.208 | 43.915 | β | -3.124 | -3.641 | β |
| Bica et al. | 2019 | 311.211 | 43.92 | β | β | β | β |
| Kharchenko et al. | 2016 | 311.192 | 43.885 | β | β | β | β |
| Kharchenko et al. | 2013 | 311.197 | 43.888 | β | -2.12 | -3.36 | β |
| Froebrich et al. | 2007 | 311.208 | 43.915 | β | β | β | β |
| Dias et al. | 2002 | 311.208 | 43.915 | β | 21.47 | -23.72 | β |
π‘ 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 1.24 | 5.16 | 2.69 | 200 | 0.170 | 414 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 784(1) | β | β |
| Cavallo et al. | 2024 | 2.57 | 4.74 | β | 115 | 0.170 | β | β | β |
| Hunt & Reffert | 2023 | 2.46 | 4.80 | 2.69 | 56 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 200 | β | 43 | β | β |
| Kharchenko et al. | 2016 | 1.24 | 5.16 | β | 200 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.24 | 5.16 | β | 200 | β | β | β | β |
| Dias et al. | 2002 | 1.24 | 5.16 | β | 200 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G80, along with HSC_659 and HSC_653.
Cavallo et al. (2024)
Gold sample.