NGC 1790

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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 10 9.1
Summary

NGC 1790 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above 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 at least one entry reported in the same catalogue.

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
Loktin & Popova (2017) 77.76 52.118 – -0.528 -0.372 –
           
UCC 77.747 52.105 0.22 -0.065 0.1 -21.823
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

NGC 1790 UCC

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Fundamental parameters

Reference Values
Loktin & Popova (2017) E(B-V)=0.558, Dist=2932, logt=9.05

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LP 55A 8.0 78.01 52.46 0.21 0.1 0.1 – 0.08