Dolidze 25
(MWSC 975)
0.69
UTI
0.46
CN
1.0
Cdens
0.25
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.46 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.25 Low quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Dolidze 25 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Massive
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 | 101.27 | 0.237 | 0.212 | -0.354 | 0.277 | â |
| Hunt & Reffert | 2024 | 101.267 | 0.228 | 0.201 | -0.328 | 0.263 | 53.822 |
| Cavallo et al. | 2024 | 101.218 | 0.269 | 0.205 | â | â | â |
| He et al. | 2023 | 101.194 | 0.318 | 0.198 | -0.364 | 0.256 | 57.96 |
| Hunt & Reffert | 2023 | 101.267 | 0.228 | 0.201 | -0.328 | 0.263 | 53.822 |
| Just et al. | 2023 | 101.273 | 0.242 | â | â | â | â |
| Jaehnig et al. | 2021 | 101.269 | 0.266 | 0.209 | -0.267 | 0.231 | â |
| Loktin & Popova | 2017 | 101.28 | 0.24 | â | -0.031 | -1.217 | 77.4 |
| Kharchenko et al. | 2016 | 101.273 | 0.242 | â | â | â | â |
| Dias et al. | 2014 | 101.275 | 0.3 | â | -0.29 | -1.79 | â |
| Kharchenko et al. | 2013 | 101.28 | 0.24 | â | 0.7 | -2.31 | 77.4 |
| Gozha et al. | 2012 | 101.275 | 0.3 | â | â | â | â |
| Kharchenko et al. | 2007 | 101.28 | 0.3 | â | 0.17 | â | â |
| van den Bergh | 2006 | 101.275 | 0.3 | â | â | â | â |
| Chen et al. | 2003 | 101.232 | 0.325 | â | 1.81 | -1.98 | 71.0 |
| Dias et al. | 2002 | 101.275 | 0.3 | â | -0.29 | -1.79 | 71.0 |
| Dambis | 1999 | 101.275 | 0.3 | 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 | 1731* | â | â |
| Cavallo et al. | 2024 | 3.72 | 1.84 | â | 83 | 0.230 | â | â | â |
| He et al. | 2023 | 3.89 | 2.25 | â | 20 | â | â | â | â |
| Hunt & Reffert | 2023 | 4.43 | 1.64 | 2.53 | 77 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 6 | â | 413 | â | â |
| Jaehnig et al. | 2021 | 4.92* | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 5.56 | 2.09 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.80 | 2.06 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.80 | 2.06 | â | 6 | â | â | â | â |
| Gozha et al. | 2012 | 6.80 | â | â | 6 | â | â | â | â |
| van den Bergh | 2006 | 6.30 | 2.23 | â | 7 | â | â | â | â |
| Chen et al. | 2003 | 6.30 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 6.80 | 2.48 | â | 6 | â | â | â | â |
| Dambis | 1999 | 2.99 | 2.24 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.