Gulliver 44

(FoF 2148)

N_50

r_50

165

9.2

Summary

Gulliver 44 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Cantat-Gaudin et al. (2018)	127.249	-38.095	0.785	-0.666	2.301	–
Soubiran et al. (2018)	127.249	-38.095	–	–	–	15.45
Bossini et al. (2019)	127.249	-38.095	–	–	–	–
Liu & Pang (2019)	127.24	-38.105	0.789	-0.699	2.289	–
Cantat-Gaudin et al. (2020)	127.249	-38.095	0.785	-0.666	2.301	–
Dias et al. (2021)	127.231	-38.099	0.782	-0.646	2.304	14.738
Tarricq et al. (2022)	127.282	-38.099	0.813	-0.638	2.372	–
He et al. (2022)	127.214	-38.087	0.811	-0.634	2.359	–
Hunt & Reffert (2023)	127.279	-38.114	0.81	-0.648	2.339	12.472
Cavallo et al. (2024)	127.224	-38.097	0.806	–	–	–
Hunt & Reffert (2024)	127.279	-38.114	0.81	-0.648	2.339	12.472
Almeida et al. (2025)	127.231	-38.099	–	–	–	–

UCC	127.25	-38.09	0.806	-0.642	2.35	14.636

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Cantat-Gaudin et al. (2018)	`dmode=1228.2`
Soubiran et al. (2018)	`dmode=1228.2`
Bossini et al. (2019)	`AV=0.502, Dist=9.925, logA=9.182, Fe/H=0.0`
Liu & Pang (2019)	`Age=0.562, Z=0.5`
Cantat-Gaudin et al. (2020)	`AVNN=0.78, DistPc=1227.0, AgeNN=8.65`
Dias et al. (2021)	`Av=1.207, Dist=1155, logage=9.007, [Fe/H]=0.102`
Tarricq et al. (2022)	`Dist=1187, logAgeNN=8.74`
He et al. (2022)	`A0=1.75, logAge=8.55`
Hunt & Reffert (2023)	`AV50=1.524, diffAV50=2.302, MOD50=10.331, logAge50=8.427`
Cavallo et al. (2024)	`AV50=1.65, dMod50=10.52, logAge50=8.51, [Fe/H]50=0.25`
Hunt & Reffert (2024)	`MassJ=572.182, MassTot=581.994`
Almeida et al. (2025)	`AV=1.207, Dist=1155, logAge=9.007, MassRk=455.4`

Search coordinates in Bayestar19

Cluster region map