FSR 0416
(MWSC 3689)
0.78
UTI
0.69
CN
1.0
Cdens
1.0
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
12.6 [N/pc2]
- CN 0.69 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0416 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a large 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 | 345.387 | 62.989 | 1.177 | -1.002 | -2.319 | -18.498 |
| Hunt & Reffert | 2024 | 345.478 | 63.005 | 1.181 | -0.98 | -2.352 | -46.659 |
| Cavallo et al. | 2024 | 345.431 | 63.014 | 1.181 | β | β | β |
| Hunt & Reffert | 2023 | 345.478 | 63.005 | 1.181 | -0.98 | -2.352 | -46.659 |
| Just et al. | 2023 | 345.518 | 63.061 | β | β | β | β |
| SΓ‘nchez et al. | 2020 | 345.571 | 63.063 | β | -2.158 | -3.19 | β |
| Kharchenko et al. | 2016 | 345.518 | 63.061 | β | β | β | β |
| Dias et al. | 2014 | 345.571 | 63.063 | β | -0.05 | -1.47 | β |
| Kharchenko et al. | 2013 | 345.525 | 63.065 | β | -1.49 | -0.09 | β |
| Kharchenko et al. | 2012 | 345.525 | 63.065 | β | -1.49 | -0.09 | β |
| Froebrich et al. | 2007 | 345.571 | 63.063 | β | β | β | β |
| Dias et al. | 2002 | 345.571 | 63.063 | β | -0.05 | -1.47 | 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 | 0.7 | 1.71 | 0.43 | 71 | 0.200 | 54 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 101(1) | β | β |
| Cavallo et al. | 2024 | 0.84 | 2.53 | β | 9 | 0.200 | β | β | β |
| Hunt & Reffert | 2023 | 0.82 | 2.33 | 0.43 | 5 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 71 | β | 8 | β | β |
| Kharchenko et al. | 2016 | 0.70 | 1.71 | β | 71 | β | β | β | β |
| Kharchenko et al. | 2013 | 0.70 | 1.71 | β | 71 | β | β | β | β |
| Kharchenko et al. | 2012 | 0.70 | 1.71 | β | 71 | β | β | β | β |
| Dias et al. | 2002 | 0.70 | 1.71 | β | 71 | 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 G82, along with Theia_4, HSC_862, UBC_178, HSC_892, ASCC_125 and UPK_198.
Cavallo et al. (2024)
Gold sample.