Sco OB5
0.55
UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
7.0 [N/pc2]
- CN 0.5 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Sco OB5 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close* distance, below the mid-plane, affected by low extinction. It is catalogued as an extremely massive, very young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~1.22 kpc) differs significantly from the median photometric distance (~3.31 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 268.109 | -38.704 | 0.817 | 2.902 | -1.812 | -14.824 |
| He et al. | 2023 | 268.137 | -38.728 | 0.804 | 2.884 | -1.796 | -17.98 |
| Piskunov et al. | 2008 | 268.129 | -38.644 | â | â | â | â |
| Piskunov et al. | 2007 | 268.129 | -38.644 | â | â | â | â |
| Kharchenko et al. | 2005 | 268.14 | -38.64 | â | 2.46 | -1.8 | 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 | 3.31 | 0.71 | â | 7 | â | 349626 | â | â |
| He et al. | 2023 | 1.29 | 1.00 | â | 16 | â | â | â | â |
| Piskunov et al. | 2008 | 3.31 | 0.71 | â | 7 | â | 588844(1) | â | â |
| Piskunov et al. | 2007 | 3.31 | 0.71 | â | 7 | â | 110408 | â | â |
| Kharchenko et al. | 2005 | 3.31 | 0.71 | â | 7 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
