Dias 3
(MWSC 1135)
0.19
UTI
0.0
CN
0.05
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
6.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.05 Very loose
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
Dias 3 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~4.13 kpc) differs significantly from the median photometric distance (~7.24 kpc).
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
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.
Very distant
Moderate extinction
Massive
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 107.615 | -8.441 | 0.242 | -1.141 | 1.505 | 83.291 |
| Just et al. | 2023 | 107.589 | -8.393 | â | â | â | â |
| Kharchenko et al. | 2016 | 107.589 | -8.393 | â | â | â | â |
| Dias et al. | 2014 | 107.629 | -8.428 | â | 1.67 | -2.33 | â |
| Kharchenko et al. | 2013 | 107.595 | -8.395 | â | 3.99 | -1.22 | â |
| Dias et al. | 2002 | 107.629 | -8.428 | â | 1.67 | -2.33 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 305 | â | 1858 | â | â |
| Kharchenko et al. | 2016 | 7.24 | 1.94 | â | 305 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.24 | 1.94 | â | 305 | â | â | â | â |
| Dias et al. | 2002 | 4.65 | 1.98 | â | 1413 | â | â | â | â |
