Collinder 458
(Harvard 21; MWSC 3774; OCL 273)
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.12 Very low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
Collinder 458 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature. (*): The parallax distance estimate (~3.92 kpc) differs significantly from the median photometric distance (~2.50 kpc).
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 | – | 358.623 | 61.78 | 0.255 | -3.031 | -1.092 | -97.6 |
| Just et al. | 2023 | 358.547 | 61.736 | – | – | – | – |
| Bica et al. | 2019 | 358.571 | 61.735 | – | – | – | – |
| Kharchenko et al. | 2016 | 358.547 | 61.736 | – | – | – | – |
| Kharchenko et al. | 2013 | 358.555 | 61.74 | – | 0.05 | -3.47 | – |
| Kharchenko et al. | 2012 | 358.555 | 61.74 | – | 0.05 | -3.47 | – |
| Dias et al. | 2002 | 358.525 | 61.767 | – | 4.48 | -6.37 | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | – | – | – | 150 | – | 54 | – | – |
| Kharchenko et al. | 2016 | 2.50 | 3.41 | – | 150 | – | – | – | – |
| Kharchenko et al. | 2013 | 2.50 | 3.41 | – | 150 | – | – | – | – |
| Kharchenko et al. | 2012 | 2.50 | 3.41 | – | 150 | – | – | – | – |
| Dias et al. | 2002 | 1.94 | 2.63 | – | 178 | – | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
