Collinder 92
(MWSC 850; OCL 504)
0.25
UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.38 Low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
Collinder 92 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~14.53 kpc) differs significantly from the median photometric distance (~2.83 kpc).
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 95.715 | 5.093 | 0.069 | 0.111 | -0.289 | 94.768 |
| He et al. | 2023 | 95.726 | 5.069 | 0.149 | 0.2 | -0.002 | 70.42 |
| Just et al. | 2023 | 95.723 | 5.101 | – | – | – | – |
| Donor et al. | 2020 | 95.73 | 5.1 | – | -0.04 | 0.23 | 84.9 |
| Bica et al. | 2019 | 95.717 | 5.134 | – | – | – | – |
| Loktin & Popova | 2017 | 95.73 | 5.118 | – | -0.67 | -2.12 | – |
| Kharchenko et al. | 2016 | 95.723 | 5.101 | – | – | – | – |
| Kharchenko et al. | 2013 | 95.73 | 5.1 | – | -1.58 | -0.73 | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| He et al. | 2023 | 5.13 | 1.50 | – | 158 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 1396 | – | 1117 | – | – |
| Donor et al. | 2020 | – | – | – | – | -0.420 | – | – | – |
| Loktin & Popova | 2017 | 2.99 | 0.90 | – | 2460 | – | – | – | – |
| Kharchenko et al. | 2016 | 2.67 | 1.62 | – | 1396 | – | – | – | – |
| Kharchenko et al. | 2013 | 2.67 | 1.62 | – | 1396 | – | – | – | – |
💡 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.
