FSR 1298
(MWSC 1377)
0.16
UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
2.4 [pc], 0.3 [pc-2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.38 Low quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
FSR 1298 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 118.384 | -22.421 | 0.258 | -2.703 | 2.474 | 78.887 |
| Hunt & Reffert | 2024 | 118.372 | -22.431 | 0.273 | -2.66 | 2.5 | 88.788 |
| Cavallo et al. | 2024 | 118.387 | -22.472 | 0.27 | â | â | â |
| Hunt & Reffert | 2023 | 118.372 | -22.431 | 0.273 | -2.66 | 2.5 | 88.788 |
| Just et al. | 2023 | 118.411 | -22.32 | â | â | â | â |
| Bica et al. | 2019 | 118.417 | -22.342 | â | â | â | â |
| Kharchenko et al. | 2016 | 118.411 | -22.32 | â | â | â | â |
| Kharchenko et al. | 2013 | 118.417 | -22.323 | â | -2.19 | -0.12 | â |
| Froebrich et al. | 2007 | 118.412 | -22.339 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.01 | 0.82 | 1.66 | 290 | -0.160 | 119 | â | â |
| Hunt & Reffert | 2024 | 3.16 | 0.69 | 1.66 | 622 | â | 99(1) | â | â |
| Cavallo et al. | 2024 | 3.01 | 0.82 | â | 309 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 3.16 | 0.69 | 1.66 | 622 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 272 | â | 139 | â | â |
| Kharchenko et al. | 2016 | 2.09 | 1.97 | â | 272 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.09 | 1.97 | â | 272 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.70 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.70 (50th percentile).