NGC 7352

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.01 0.25 0.0 1.0
C3
N_50
r_50
CC 11 8.2
Summary

NGC 7352 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.

This object shares a very small percentage of members with a later reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 339.929 57.395 – 0.25 -3.46 –
Loktin & Popova (2017) 339.93 57.395 – -0.685 -0.843 –
           
UCC 339.977 57.38 0.159 -2.851 -1.774 -87.292
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

NGC 7352 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.1, Dist=2550.0, Age=7.7
Loktin & Popova (2017) E(B-V)=0.171, Dist=3245, logt=8.98

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1169 8.0 340.08 57.09 0.19 -2.83 -1.73 -96.99 0.51