Dolidze 38
(MWSC 3251)
0.28
UTI
0.39
CN
0.0
Cdens
0.38
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
39
Core radius and density
4.4 [pc], 0.02 [pc-2]
- CN 0.39 Poorly populated
- Cdens 0.0 Very loose
- CC3 0.38 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Dolidze 38 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~7.91 kpc) differs significantly from the median photometric distance (~1.53 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 301.484 | 41.177 | 0.126 | -3.016 | -3.466 | -28.186 |
| Just et al. | 2023 | 301.465 | 41.193 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -3.37 | -4.17 | â |
| Dib et al. | 2018 | 301.47 | 41.195 | â | â | â | â |
| Loktin & Popova | 2017 | 301.425 | 41.2 | â | -0.675 | -0.348 | â |
| Sampedro et al. | 2017 | 301.425 | 41.2 | â | -1.95 | -7.0 | â |
| Joshi et al. | 2016 | 301.47 | 41.195 | â | â | â | â |
| Kharchenko et al. | 2016 | 301.465 | 41.193 | â | â | â | â |
| Dias et al. | 2014 | 301.425 | 41.2 | â | -1.73 | -6.11 | â |
| Kharchenko et al. | 2013 | 301.47 | 41.195 | â | -2.82 | -1.41 | â |
| Piskunov et al. | 2008 | 301.389 | 41.196 | â | â | â | â |
| Kharchenko et al. | 2005 | 301.39 | 41.2 | â | -3.59 | -6.49 | â |
| Dias et al. | 2002 | 301.425 | 41.2 | â | -1.73 | -6.11 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.53 | 0.72 | â | 1462 | â | 352 | â | â |
| Just et al. | 2023 | â | â | â | 1462 | â | 403 | â | â |
| Dib et al. | 2018 | 1.53 | â | â | 1462 | â | â | â | â |
| Loktin & Popova | 2017 | 3.29 | 0.73 | â | 2239 | â | â | â | â |
| Joshi et al. | 2016 | 1.53 | 0.72 | â | 1462 | â | 302 | â | â |
| Kharchenko et al. | 2016 | 1.53 | 0.72 | â | 1462 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.53 | 0.72 | â | 1462 | â | â | â | â |
| Piskunov et al. | 2008 | 1.20 | 0.47 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.20 | 0.47 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 1.20 | 0.47 | â | 891 | â | â | â | â |
MOCA

Bica et al. (2019)
Analysis of Dolidze objects by M. Kronberger reported in DAML02. Asterisms and cluster alikes by B. Alessi reported in DAML02.