Dolidze 42
(MWSC 3313)
0.35
UTI
0.0
CN
0.18
Cdens
0.38
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
15.3 [arcmin]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.38 Low quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Dolidze 42 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 304.981 | 38.097 | 0.869 | -2.968 | -7.319 | 10.151 |
| Hunt & Reffert | 2024 | 304.904 | 38.099 | 0.87 | -2.995 | -7.358 | 15.193 |
| Cavallo et al. | 2024 | 304.936 | 38.064 | 0.867 | â | â | â |
| Hunt & Reffert | 2023 | 304.904 | 38.099 | 0.87 | -2.995 | -7.358 | 15.193 |
| Just et al. | 2023 | 304.9 | 38.139 | â | â | â | â |
| Loktin & Popova | 2017 | 304.92 | 38.133 | â | -0.976 | -1.265 | â |
| Kharchenko et al. | 2016 | 304.9 | 38.139 | â | â | â | â |
| Dias et al. | 2014 | 304.925 | 38.133 | â | -1.14 | -0.53 | â |
| Kharchenko et al. | 2013 | 304.905 | 38.141 | â | -4.22 | -4.2 | â |
| van den Bergh | 2006 | 304.925 | 38.133 | â | â | â | â |
| Dias et al. | 2002 | 304.925 | 38.133 | â | -1.14 | -0.53 | 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 | 86* | â | â |
| Cavallo et al. | 2024 | 1.16 | 1.69 | â | 9 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 1.10 | 1.41 | 1.60 | 8 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 33 | â | 23 | â | â |
| Loktin & Popova | 2017 | 0.98 | 1.76 | â | 37 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.24 | 1.29 | â | 33 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.24 | 1.29 | â | 33 | â | â | â | â |
| van den Bergh | 2006 | 0.97 | 1.77 | â | 35 | â | â | â | â |
| Dias et al. | 2002 | 0.97 | 1.77 | â | 35 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.