NGC 7084
(MWSC 3524)
0.18
UTI
0.26
CN
0.02
Cdens
0.25
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
26
Core radius and density
4.0 [pc], 0.08 [pc-2]
- CN 0.26 Poorly populated
- Cdens 0.02 Very loose
- CC3 0.25 Low quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
NGC 7084 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.
(*): The parallax distance estimate (~3.06 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 | 323.041 | 17.58 | 0.327 | -5.887 | -7.365 | 6.133 |
| Bica et al. | 2019 | 322.952 | 17.418 | â | â | â | â |
| Dib et al. | 2018 | 323.055 | 17.575 | â | â | â | â |
| Loktin & Popova | 2017 | 323.055 | 17.572 | â | -2.76 | -10.027 | â |
| Sampedro et al. | 2017 | 323.137 | 17.508 | â | -1.65 | -6.81 | â |
| Joshi et al. | 2016 | 323.055 | 17.575 | â | â | â | â |
| Tadross | 2014 | 323.137 | 17.508 | â | â | â | â |
| Dias et al. | 2014 | 323.137 | 17.508 | â | -1.39 | -6.76 | â |
| Dias et al. | 2002 | 323.137 | 17.508 | â | -1.39 | -6.76 | 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 | 0.32 | â | 1514 | â | â | â | â |
| Dib et al. | 2018 | 1.26 | â | â | 2661 | â | â | â | â |
| Loktin & Popova | 2017 | 2.41 | 0.71 | â | 708 | â | â | â | â |
| Joshi et al. | 2016 | 1.26 | 0.00 | â | 2661 | â | â | â | â |
| Tadross | 2014 | 0.77 | 0.32 | â | 1500 | â | â | â | â |
| Dias et al. | 2002 | 0.77 | 0.32 | â | 1514 | â | â | â | â |
MOCA

Cantat-Gaudin & Anders (2020)
Marked non-existent. Proper-motion analysis confirms lack of a physical cluster. More details in Appendix A of the article.
Bica et al. (2019)
Original NGC and IC catalogues at Vizier: NGC 2000.0, Sky Publishing, ed. Sinnott 1988 (1997yCat.7118....0S).