VVVX CL100
0.00
UTI
0.44
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.44 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 0.0 Very likely duplicate
Overview
VVVX CL100 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 8 years.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.
No fundamental parameters
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 274.685 | -13.825 | 0.542 | 0.162 | -1.774 | -16.275 |
| Borissova et al. | 2018 | 274.718 | -13.859 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
Borissova et al. (2018)
Four bright stars, very compact, part of M16, RSG?.