LP 24

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C3
N_50
r_50
CC 31 4.0
Summary

LP 24 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.

This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.94) 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) 332.625 57.886 -3.906 -2.293
           
UCC 332.614 57.855 0.199 -2.854 -1.787
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

LP 24 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Loktin & Popova (2017) E(B-V)=0.542, Dist=2301, logt=7.72

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3072 16.1 332.61 57.74 0.16 -2.86 -2.02 0.03
HSC 796 12.9 332.63 57.74 0.16 -2.86 -2.02 -58.94 0.06
FSR 0354 6.5 332.75 57.69 0.17 -2.89 -2.03 -48.45 0.39