Cmg 119
0.56
UTI
0.29
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
3.3 [arcmin]
- CN 0.29 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Cmg 119 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.74 kpc) differs significantly from the median photometric distance (~1.36 kpc).
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 88.416 | -10.409 | 1.343 | -1.313 | 1.799 | 25.115 |
| Hunt & Reffert | 2024 | 88.415 | -10.394 | 1.325 | -1.254 | 1.877 | 27.696 |
| Cavallo et al. | 2024 | 88.383 | -10.436 | 1.32 | â | â | â |
| Hunt & Reffert | 2023 | 88.415 | -10.394 | 1.325 | -1.254 | 1.877 | 27.696 |
| Bica et al. | 2019 | 88.424 | -10.402 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 91* | â | â |
| Cavallo et al. | 2024 | 2.00 | 2.12 | â | 18 | -0.270 | â | â | â |
| Hunt & Reffert | 2023 | 0.73 | 3.20 | 1.89 | 6 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Wood sample.