LS 139

(La Serena 139)

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.66 0.12 0.0 0.96
C3
N_50
r_50
DC 23 3.5
Summary

LS 139 is a sparse, moderately dense object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.This is a unique object, which shares a very small percentage of members with at least one previously 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=0.96) 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
Bica et al. (2019) 211.501 -61.589 – – – –
           
UCC 211.523 -61.574 0.385 -7.465 -2.602 -22.874
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

LS 139 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVV 035 4.0 211.61 -61.45 0.35 -7.69 -2.83 -51.93 0.14