Melotte 110

(Collinder 255; VDBH 130; NGC 4349; MWSC 2024; OCL 882; vdBergh-Hagen 130; ESO 131 03; FSR 1614; FoF 422)

1.0 UTI

1.0

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 944

Stellar density (N₅₀/rad) 96.0 [N/pc²]

C3 classification AA

C_N 1.0 Very rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Melotte 110 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Massive Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Melotte 110 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–	186.056	-61.863	0.519	-7.845	-0.264	-12.561
Li et al.	2025	186.048	-61.866	0.49	-7.827	-0.296	–
Hu & Soubiran	2025	186.062	-61.863	–	–	–	–
Almeida et al.	2025	186.047	-61.869	–	–	–	–
Hunt & Reffert	2024	186.055	-61.864	0.524	-7.841	-0.258	-14.223
Cavallo et al.	2024	186.062	-61.863	0.525	–	–	–
Hunt & Reffert	2023	186.055	-61.864	0.524	-7.841	-0.258	-14.223
Just et al.	2023	186.051	-61.866	–	–	–	–
Jaehnig et al.	2021	186.058	-61.862	0.529	-7.832	-0.304	–
Rain et al.	2021	186.048	-61.866	0.49	-7.827	-0.296	–
Dias et al.	2021	186.047	-61.869	0.491	-7.825	-0.298	-11.773
Cantat-Gaudin et al.	2020	186.048	-61.866	0.49	-7.827	-0.296	–
Sánchez et al.	2020	186.033	-61.872	–	-7.828	-0.292	–
Cantat-Gaudin & Anders	2020	186.048	-61.866	0.49	-7.827	-0.296	–
Liu & Pang	2019	186.055	-61.858	0.493	-7.787	-0.249	–
Bossini et al.	2019	186.048	-61.866	–	–	–	–
Soubiran et al.	2018	186.048	-61.866	–	–	–	-11.46
Bica et al.	2019	186.033	-61.881	–	–	–	–
Cantat-Gaudin et al.	2018	186.048	-61.866	0.49	-7.827	-0.296	–
Loktin & Popova	2017	186.03	-61.872	–	-12.378	-4.928	-15.0
Kharchenko et al.	2016	186.051	-61.866	–	–	–	–
Dias et al.	2014	186.033	-61.872	–	-1.9	-0.16	–
Kharchenko et al.	2013	186.06	-61.87	–	-9.57	-1.75	-15.0
Gozha et al.	2012	186.033	-61.872	–	–	–	–
Piskunov et al.	2008	186.058	-61.862	–	–	–	–
Kharchenko et al.	2007	186.03	-61.87	–	0.22	–	-15.69
Piskunov et al.	2007	186.058	-61.862	–	–	–	–
van den Bergh	2006	186.05	-61.867	–	–	–	–
Kharchenko et al.	2005	186.06	-61.87	–	-6.41	0.33	-15.69
Kharchenko et al.	2003	186.07	-61.88	–	-6.31	0.67	–
Chen et al.	2003	186.011	-61.88	–	–	–	–
Dias et al.	2002	186.033	-61.872	–	-5.77	1.44	-11.87

💡 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–	1.99	1.18	0.57	257	-0.120	2481	–	0.0
Li et al.	2025	1.61	1.04	–	600	-0.150	–	–	–
Hu & Soubiran	2025	–	–	–	–	-0.300⁽⁵⁾	–	–	–
Almeida et al.	2025	1.66	1.30	–	342	–	767	–	–
Hunt & Reffert	2024	–	–	–	–	–	4106⁽¹⁾	–	–
Cavallo et al.	2024	1.55	1.24	–	525	-0.190	–	–	–
Hunt & Reffert	2023	1.79	0.86	0.57	352	–	–	–	–
Just et al.	2023	–	–	–	257	–	1186	–	–
Jaehnig et al.	2021	1.88⁽¹⁾	–	–	–	–	–	–	–
Rain et al.	2021	1.93	1.15	–	282	–	–	–	0
Dias et al.	2021	1.66	1.30	–	342	-0.034	–	–	–
Cantat-Gaudin et al.	2020	1.92	1.01	–	316	–	–	–	–
Cantat-Gaudin & Anders	2020	1.93	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	977	-2.000	–	–	–
Bossini et al.	2019	1.99	1.16	–	282	-0.070	–	–	–
Soubiran et al.	2018	1.93	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	1.93	–	–	–	–	–	–	–
Loktin & Popova	2017	2.18	1.17	–	212	–	–	–	–
Kharchenko et al.	2016	2.15	1.39	–	257	–	–	–	–
Kharchenko et al.	2013	2.15	1.39	–	257	0.105	–	–	–
Gozha et al.	2012	2.18	–	–	207	-0.120	4365	–	–
Piskunov et al.	2008	2.18	1.18	–	209	–	3776⁽¹⁾	–	–
Piskunov et al.	2007	2.18	1.18	–	209	–	637	–	–
van den Bergh	2006	2.18	1.18	–	209	–	–	–	–
Kharchenko et al.	2005	2.18	1.18	–	209	–	–	–	–
Kharchenko et al.	2003	2.18	1.18	–	–	–	–	–	–
Chen et al.	2003	2.18	1.19	–	200	-0.120⁽¹⁾	–	–	–
Dias et al.	2002	2.18	1.19	–	207	-0.120	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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