NGC 7036
0.18
UTI
0.0
CN
0.06
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
0.3 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.12 Very low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 7036 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.
(*): The parallax distance estimate (~5.03 kpc) differs significantly from the median photometric distance (~1.08 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 | 317.495 | 15.519 | 0.199 | -3.334 | -5.641 | -33.245 |
| Angelo et al. | 2019 | 317.492 | 15.514 | â | â | â | â |
| Loktin & Popova | 2017 | 317.505 | 15.517 | â | 1.44 | -5.68 | â |
| Bukowiecki et al. | 2011 | 317.492 | 15.527 | â | â | â | â |
| van den Bergh | 2006 | 317.508 | 15.518 | â | â | â | â |
| Dias et al. | 2002 | 317.508 | 15.517 | â | 1.44 | -5.68 | 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 | 1.08 | 0.185 | â | 3162 | â | 22 | â | â |
| Angelo et al. | 2019 | 1.46 | â | â | 2240 | â | 15 | â | â |
| Loktin & Popova | 2017 | 1.38 | 0.06 | â | 2163 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 28 | â | â |
| Bukowiecki et al. | 2011 | 1.08(1) | 0.00 | â | 3981 | â | â | â | â |
| van den Bergh | 2006 | 1.00 | 0.31 | â | 3162 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.31 | â | 3162 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Cantat-Gaudin & Anders (2020)
Flagged as non-existent; Gaia DR2 data show no coherent kinematic group despite proposed members. More details in Appendix A of the article.