NGC 7429

(OCL 249; MWSC 3676)

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.78 1.0 1.0 0.5 1.0
C3
N_50
r_50
AA 170 42.0
Summary

NGC 7429 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It is moderately studied in the literature.

This object shares a large percentage of members with 3 later reported entries.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 344.0 59.973 – 0.22 -0.03 –
Kharchenko et al. (2012) 343.973 59.96 – -2.59 2.38 –
Loktin & Popova (2017) 343.965 59.956 – -0.7 0.283 –
Bica et al. (2019) 344.019 59.965 – – – –
Hunt & Reffert (2023) 344.09 59.912 2.371 4.771 -2.245 -12.037
Cavallo et al. (2024) 344.019 59.87 2.373 – – –
           
UCC 344.027 59.884 2.359 4.811 -2.189 -12.685
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

NGC 7429 UCC
NGC 7429 HUNT23

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.16, Dist=1190.0, Age=7.6
Kharchenko et al. (2012) e_bv=0.949, distance=1250, log_age=8.08
Loktin & Popova (2017) E(B-V)=0.6, Dist=1735, logt=8.3
Hunt & Reffert (2023) AV50=0.448, diffAV50=0.396, MOD50=8.015, logAge50=7.893
Cavallo et al. (2024) AV50=0.77, dMod50=8.21, logAge50=7.85, [Fe/H]50=0.31

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
RSG7 76.5 344.32 59.45 2.25 5.18 -1.78 -11.08 0.49
RSG8 68.2 345.08 59.41 2.17 5.45 -1.65 -10.45 0.8
CWWDL 14637 30.0 343.95 59.81 2.37 4.78 -2.24 -12.62 0.0