Cyg OB2
0.15
UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.13
Clit
0.25
Cdup
Stellar density (N50/rad)
45.4 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.13 Rarely studied
- Cdup 0.25 Possibly duplicate
Overview
Cyg OB2 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as an extremely massive, very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously 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 | 308.307 | 41.3 | 0.58 | -2.72 | -4.407 | -8.189 |
| Dib et al. | 2018 | 308.317 | 41.32 | â | â | â | â |
| Joshi et al. | 2016 | 308.317 | 41.32 | â | â | â | â |
| Piskunov et al. | 2008 | 308.299 | 41.304 | â | â | â | â |
| Kharchenko et al. | 2007 | 308.1 | 41.28 | â | 0.6 | â | -28.0 |
| Piskunov et al. | 2007 | 308.299 | 41.304 | â | â | â | â |
| Kharchenko et al. | 2005 | 308.31 | 41.31 | â | -1.6 | -4.72 | -28.0 |
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 | 1.5 | 4.1 | â | 5 | â | 25645 | â | â |
| Dib et al. | 2018 | 1.59 | â | â | 5 | â | â | â | â |
| Joshi et al. | 2016 | 1.59 | 5.78 | â | 5 | â | 30903 | â | â |
| Piskunov et al. | 2008 | 1.50 | 4.10 | â | 5 | â | 25645(1) | â | â |
| Piskunov et al. | 2007 | 1.50 | 4.10 | â | 5 | â | 3532 | â | â |
| Kharchenko et al. | 2005 | 1.50 | 4.10 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
