Dolidze 28
(MWSC 2913)
0.19
UTI
0.0
CN
0.05
Cdens
0.25
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
15
Core radius and density
2.0 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.25 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Dolidze 28 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~2.53 kpc) differs significantly from the median photometric distance (~1.26 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 276.378 | -14.665 | 0.395 | -1.716 | -2.709 | â |
| Just et al. | 2023 | 276.363 | -14.651 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -0.23 | -2.56 | â |
| Dib et al. | 2018 | 276.37 | -14.65 | â | â | â | â |
| Loktin & Popova | 2017 | 276.375 | -14.656 | â | -0.305 | -3.775 | 0.6 |
| Sampedro et al. | 2017 | 276.371 | -14.656 | â | -1.12 | -0.71 | â |
| Joshi et al. | 2016 | 276.37 | -14.65 | â | â | â | â |
| Kharchenko et al. | 2016 | 276.363 | -14.651 | â | â | â | â |
| Dias et al. | 2014 | 276.371 | -14.656 | â | 0.17 | -1.47 | 0.6 |
| Kharchenko et al. | 2013 | 276.37 | -14.65 | â | 0.67 | -3.58 | 0.6 |
| Morales et al. | 2013 | 276.371 | -14.656 | â | â | â | â |
| Dias et al. | 2002 | 276.371 | -14.656 | â | 0.17 | -1.47 | 0.6 |
| Lynga | 1987 | 276.345 | -14.649 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.26 | 2.96 | â | 178 | â | 91 | â | â |
| Just et al. | 2023 | â | â | â | 178 | â | 91 | â | â |
| Dib et al. | 2018 | 1.26 | â | â | 178 | â | â | â | â |
| Loktin & Popova | 2017 | 4.79 | 5.09 | â | 25 | â | â | â | â |
| Joshi et al. | 2016 | 1.26 | 2.96 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.26 | 2.96 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.26 | 2.96 | â | 178 | â | â | â | â |
| Dias et al. | 2002 | 1.26 | 2.96 | â | 178 | â | â | â | â |
MOCA

Bica et al. (2019)
Analysis of Dolidze objects by M. Kronberger reported in DAML02.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: one or a few submm emission within the cluster area.