LS 474

(La Serena 474)

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C3
N_50
r_50
DC 157 9.3
Summary

LS 474 is a rich, very dense object of very low C3 quality. It is located at a relatively close 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 very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Bica et al. (2019) 257.904 -38.354
           
UCC 257.881 -38.296 0.584 -2.455 -3.32 -27.477
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

LS 474 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 1755 15.3 258.1 -38.44 0.61 -2.63 -3.64 -36.13 0.18
Teutsch 258 3.2 257.85 -38.43 0.64 -2.81 -4.64 -34.03 0.09
Ryu 401 1.3 257.95 -38.61 0.66 -1.41 -3.07 -39.66 0.23