Gulliver 29

0.74 UTI

0.82

C_N

1.0

C_dens

1.0

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 282

Stellar density (N₅₀/rad) 7.3 [N/pc²]

C3 classification AA

C_N 0.82 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Gulliver 29 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Massive Near-solar metallicity Very young

Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg03' along with ASCC 88.

Data

🔍 Search references for Gulliver 29 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	256.671	-35.259	0.903	1.279	-2.204	5.004
Celli et al.	2024	256.745	-35.205	–	–	–	–
He et al.	2022	256.744	-35.478	0.903	1.261	-2.274	–
Spina et al.	2021	256.749	-35.197	0.899	1.314	-2.19	–
Cantat-Gaudin et al.	2020	256.745	-35.205	0.905	1.325	-2.206	–
Cantat-Gaudin & Anders	2020	256.745	-35.205	0.905	1.325	-2.206	–
Monteiro & Dias	2019	256.745	-35.205	–	–	–	2.144
Soubiran et al.	2018	256.745	-35.205	–	–	–	3.46
Cantat-Gaudin et al.	2018	256.745	-35.205	0.905	1.325	-2.206	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	1.07	2.0	–	11	0.006	1591	–	–
Celli et al.	2024	–	–	–	11	–	1591	–	–
He et al.	2022	–	2.00	–	9	–	–	–	–
Spina et al.	2021	1.12	–	–	11	–	–	–	–
Cantat-Gaudin et al.	2020	1.18	1.02	–	11	–	–	–	–
Cantat-Gaudin & Anders	2020	1.07	–	–	–	–	–	–	–
Monteiro & Dias	2019	0.95	2.20	–	16	0.006	–	–	–
Soubiran et al.	2018	1.07	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.07	–	–	–	–	–	–	–

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	0.11

💡 Note: The % column shows the percentage of members that Gulliver 29 shares with each listed object.

Visualization

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