Waterloo 3

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.47 0.46 0.75 0.42 1.0
C3
N_50
r_50
AB 47 3.0
Summary

Waterloo 3 is a poorly populated, loose object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is poorly studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 118.775 -25.365 – -1.18 3.41 –
Kharchenko et al. (2012) 118.767 -25.372 – -1.18 3.41 –
Hunt & Reffert (2023) 118.778 -25.358 0.197 -2.408 2.671 116.962
Cavallo et al. (2024) 118.818 -25.422 0.196 – – –
Hunt & Reffert (2024) 118.778 -25.358 0.197 -2.408 2.671 116.962
           
UCC 118.775 -25.356 0.193 -2.365 2.685 91.877
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Waterloo 3 UCC
Waterloo 3 HUNT23

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.34, Dist=5200.0
Kharchenko et al. (2012) e_bv=0.416, distance=2589, log_age=8.5
Hunt & Reffert (2023) AV50=0.429, diffAV50=1.346, MOD50=13.54, logAge50=8.45
Cavallo et al. (2024) AV50=0.76, dMod50=12.79, logAge50=8.49, [Fe/H]50=-0.2
Hunt & Reffert (2024) MassJ=356.247, MassTot=455.457

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 465 59.6 118.84 -25.42 0.19 -2.4 2.68 – 0.14