Gulliver 13

(CMa03)

N_50

r_50

100

7.5

Summary

Gulliver 13 is a rich, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, below 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)	104.858	-13.254	0.62	-2.941	0.281	–
Soubiran et al. (2018)	104.858	-13.254	–	–	–	56.53
Cantat-Gaudin et al. (2020)	104.858	-13.254	0.62	-2.941	0.281	–
Dias et al. (2021)	104.874	-13.247	0.617	-2.935	0.301	56.889
Santos-Silva et al. (2021)	104.86	-13.25	0.63	-2.92	0.31	–
Tarricq et al. (2022)	104.852	-13.249	0.623	-2.919	0.296	–
Hunt & Reffert (2023)	104.877	-13.249	0.617	-2.941	0.302	52.009
Cavallo et al. (2024)	104.869	-13.242	0.622	–	–	–
Hunt & Reffert (2024)	104.877	-13.249	0.617	-2.941	0.302	52.009
Almeida et al. (2025)	104.874	-13.247	–	–	–	–
Hu & Soubiran (2025)	104.869	-13.242	–	–	–	–

UCC	104.858	-13.256	0.626	-2.935	0.294	57.842

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=1540.4`
Soubiran et al. (2018)	`dmode=1540.4`
Cantat-Gaudin et al. (2020)	`AVNN=0.78, DistPc=1513.0, AgeNN=9.0`
Dias et al. (2021)	`Av=1.676, Dist=1501, logage=8.774, [Fe/H]=-0.05`
Santos-Silva et al. (2021)	`AVPM=1.71, AVPf=1.18, DPM=1531, DPf=1542.0, AgeM=536.0, AgeF=650, [Fe/H]M=-0.12, [Fe/H]f=0.3`
Tarricq et al. (2022)	`Dist=1466, logAgeNN=9.03`
Hunt & Reffert (2023)	`AV50=1.331, diffAV50=2.225, MOD50=10.85, logAge50=8.778`
Cavallo et al. (2024)	`AV50=1.09, dMod50=10.71, logAge50=9.02, [Fe/H]50=0.0`
Hunt & Reffert (2024)	`MassJ=395.282, MassTot=451.651`
Almeida et al. (2025)	`AV=1.676, Dist=1501, logAge=8.774, MassRk=351.0`
Hu & Soubiran (2025)	`MA22=-0.14, MA23f=-0.26, MA23g=-0.02, MZ23=-0.11, MK24=-0.16, MF24=-0.17`

Search coordinates in Bayestar19

Cluster region map