NGC 2367

(MWSC 1178)

0.84 UTI

0.56

C_N

1.0

C_dens

0.62

C_C3

1.0

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 62

Radius (P>50% members) 2.2 [arcmin]

C_N 0.56 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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NGC 2367 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Very young

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

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for NGC 2367 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	–	110.033	-21.876	0.402	-1.689	2.538	35.639
Almeida et al.	2025	110.027	-21.864	–	–	–	–
Hunt & Reffert	2024	110.038	-21.881	0.387	-1.716	2.516	35.59
Celli et al.	2024	110.031	-21.867	–	–	–	–
Cavallo et al.	2024	110.023	-21.871	0.393	–	–	–
Hunt & Reffert	2023	110.038	-21.881	0.387	-1.716	2.516	35.59
Just et al.	2023	110.049	-21.863	–	–	–	–
Rain et al.	2021	110.031	-21.867	0.395	-1.668	2.538	–
Dias et al.	2021	110.027	-21.864	0.4	-1.72	2.51	–
Cantat-Gaudin et al.	2020	110.031	-21.867	0.395	-1.668	2.538	–
Cantat-Gaudin & Anders	2020	110.031	-21.867	0.395	-1.668	2.538	–
Cantat-Gaudin et al.	2018	110.031	-21.867	0.395	-1.668	2.538	–
Loktin & Popova	2017	110.025	-21.881	–	-4.1	1.897	45.3
Kharchenko et al.	2016	110.049	-21.863	–	–	–	–
Dias et al.	2014	110.025	-21.882	–	-2.56	-0.13	–
Kharchenko et al.	2013	110.055	-21.865	–	-5.13	3.15	45.3
Gozha et al.	2012	110.025	-21.882	–	–	–	–
Piskunov et al.	2008	110.024	-21.886	–	–	–	–
Kharchenko et al.	2007	110.02	-21.88	–	0.17	–	45.33
van den Bergh	2006	110.025	-21.883	–	–	–	–
Kharchenko et al.	2005	110.02	-21.89	–	-2.25	4.91	45.33
Kharchenko et al.	2003	110.02	-21.89	–	-2.61	5.14	–
Dias et al.	2002	110.025	-21.882	–	-2.56	-0.13	33.1
Dambis	1999	110.025	-21.882	–	–	–	–

💡 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]	Bfr	BSS
Almeida et al.	2025	1.72	1.02	–	31	–	100	–	–
Hunt & Reffert	2024	–	–	–	–	–	272*	–	–
Celli et al.	2024	–	–	–	14	–	194	–	–
Cavallo et al.	2024	2.21	1.27	–	6	-0.300	–	–	–
Hunt & Reffert	2023	2.23	1.21	1.66	16	–	–	–	–
Just et al.	2023	–	–	–	27	–	403	–	–
Rain et al.	2021	2.36	0.16	–	5	–	–	–	0
Dias et al.	2021	1.72	1.02	–	31	-0.065	–	–	–
Cantat-Gaudin et al.	2020	2.28	1.34	–	14	–	–	–	–
Cantat-Gaudin & Anders	2020	2.36	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.36	–	–	–	–	–	–	–
Loktin & Popova	2017	2.00	1.03	–	5	–	–	–	–
Kharchenko et al.	2016	1.77	1.03	–	27	–	–	–	–
Kharchenko et al.	2013	1.77	1.03	–	27	–	–	–	–
Gozha et al.	2012	1.40	–	–	5	–	1259	–	–
Piskunov et al.	2008	2.00	1.02	–	10	–	–	–	–
van den Bergh	2006	2.00	1.02	–	5	–	–	–	–
Kharchenko et al.	2005	2.00	1.02	–	10	–	–	–	–
Kharchenko et al.	2003	2.00	1.02	–	–	–	–	–	–
Dias et al.	2002	1.40	0.16	–	5	–	–	–	–
Dambis	1999	2.00	1.05	–	10	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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