NGC 7352
0.10
UTI
0.0
CN
0.0
Cdens
0.25
CC3
0.13
Clit
1.0
Cdup
Nm (P>50%)
11
Core radius and density
14 [pc], 0.02 [pc-2]
- CN 0.0 Sparse
- Cdens 0.0 Very loose
- CC3 0.25 Low quality
- Clit 0.13 Rarely studied
- Cdup 1.0 Unique
Overview
NGC 7352 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.
(*): The parallax distance estimate (~6.31 kpc) differs significantly from the median photometric distance (~2.55 kpc).
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
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 | 339.977 | 57.38 | 0.159 | -2.851 | -1.774 | -87.292 |
| Dias et al. | 2018 | â | â | â | -2.72 | -1.3 | â |
| Loktin & Popova | 2017 | 339.93 | 57.395 | â | -0.685 | -0.843 | â |
| Sampedro et al. | 2017 | 339.929 | 57.395 | â | 0.24 | -3.44 | â |
| Tadross | 2014 | 339.929 | 57.395 | â | â | â | â |
| Dias et al. | 2014 | 339.929 | 57.395 | â | 0.25 | -3.46 | â |
| Dias et al. | 2002 | 339.929 | 57.395 | â | 0.25 | -3.46 | 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 | 2.55 | 3.47 | â | 50 | â | â | â | â |
| Loktin & Popova | 2017 | 3.25 | 0.54 | â | 955 | â | â | â | â |
| Tadross | 2014 | 2.55 | 3.47 | â | 50 | â | â | â | â |
| Dias et al. | 2002 | 2.55 | 3.47 | â | 50 | â | â | â | â |
MOCA
