NGC 2467

0.44 UTI

0.0

C_N

0.05

C_dens

0.5

C_C3

0.82

C_lit

1.0

C_dup

C3 classification BB

Number of members (P>50%) 19

Radius (P>50% members) 6.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.82 Well-studied
C_dup 1.0 Unique

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

Overview

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NGC 2467 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~4.68 kpc) differs significantly from the median photometric distance (~1.35 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for NGC 2467 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	–	117.969	-26.408	0.214	-1.486	2.45	77.88
Hunt & Reffert	2024	117.997	-26.411	0.216	-1.49	2.453	77.739
Cavallo et al.	2024	117.925	-26.383	0.216	–	–	–
Hunt & Reffert	2023	117.997	-26.411	0.216	-1.49	2.453	77.739
Jaehnig et al.	2021	118.18	-26.374	0.191	-2.554	2.578	–
Loktin & Popova	2017	118.11	-26.436	–	–	–	55.8
Dias et al.	2014	118.108	-26.437	–	-3.65	2.68	–
Gozha et al.	2012	118.108	-26.437	–	–	–	–
Piskunov et al.	2008	118.059	-26.437	–	–	–	–
Kharchenko et al.	2007	118.11	-26.44	–	0.2	–	55.75
van den Bergh	2006	118.08	-26.442	–	–	–	–
Kharchenko et al.	2005	118.06	-26.44	–	-3.93	1.68	55.75
Kharchenko et al.	2003	118.08	-26.39	–	-4.41	0.45	–
Chen et al.	2003	118.088	-26.363	–	-5.82	1.63	66.0
Dias et al.	2002	118.108	-26.437	–	-3.65	2.68	58.24
Dambis	1999	118.08	-26.442	–	–	–	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	102*	–	–
Cavallo et al.	2024	3.80	0.47	–	288	0.430	–	–	–
Hunt & Reffert	2023	4.56	0.73	1.19	248	–	–	–	–
Jaehnig et al.	2021	5.17*	–	–	–	–	–	–	–
Loktin & Popova	2017	1.35	1.05	–	13	–	–	–	–
Gozha et al.	2012	1.35	–	–	13	–	631	–	–
Piskunov et al.	2008	1.35	1.05	–	112	–	–	–	–
van den Bergh	2006	1.35	1.05	–	13	–	–	–	–
Kharchenko et al.	2005	1.35	1.05	–	112	–	–	–	–
Kharchenko et al.	2003	1.35	1.05	–	–	–	–	–	–
Chen et al.	2003	1.35	–	–	10	–	–	–	–
Dias et al.	2002	1.35	1.05	–	13	–	–	–	–
Dambis	1999	1.26	0.92	–	50	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1615	76.0	117.95	-26.34	0.22	-1.48	2.44	77.88	0.03

💡 Note: The % column shows the percentage of members that NGC 2467 shares with each listed object.

Visualization

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