Gulliver 29

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.82 1.0 1.0 0.42 1.0
C3
N_50
r_50
AA 282 19.3
Summary

Gulliver 29 is a rich, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is poorly studied in the literature.

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

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Cantat-Gaudin et al. (2018) 256.745 -35.205 0.905 1.325 -2.206 –
Soubiran et al. (2018) 256.745 -35.205 – – – 3.46
Cantat-Gaudin et al. (2020) 256.745 -35.205 0.905 1.325 -2.206 –
He et al. (2022) 256.744 -35.478 0.903 1.261 -2.274 –
Celli et al. (2024) 256.745 -35.205 – – – –
           
UCC 256.671 -35.259 0.903 1.279 -2.204 5.004
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Gulliver 29 UCC
Gulliver 29 CANTAT20

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Fundamental parameters

Reference Values
Cantat-Gaudin et al. (2018) dmode=1070.9
Soubiran et al. (2018) dmode=1070.9
Cantat-Gaudin et al. (2020) AVNN=1.02, DistPc=1180.0, AgeNN=7.03
He et al. (2022) A0=2.0, logAge=6.95
Celli et al. (2024) Age=10.7, Mc=1590.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14433 38.3 256.51 -35.07 0.91 1.26 -2.17 1.46 0.0
CWWDL 14471 14.9 256.42 -35.15 0.93 1.2 -2.17 0.25 0.01
OC 0684 6.0 256.79 -35.73 0.91 1.24 -2.35 -1.29 0.12