NGC 2467

0.36 UTI

0.0

C_N

0.02

C_dens

0.5

C_C3

0.65

C_lit

1.0

C_dup

N_m (P>50%) 19

Core radius and density 4.5 [pc], 0.1 [pc^-2]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.65 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

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 moderately 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.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Ahumada & Lapasset (2007)
The dereddened colour-magnitude diagram in (1989A&AS...77..321F) was examined; the authors suggest that this is a superposition of early-type stars rather than a cluster.

Data

🔍 Search references for NGC 2467 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	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	–
Dias et al.	2018	–	–	–	-1.99	2.78	–
Loktin & Popova	2017	118.11	-26.436	–	–	–	55.8
Sampedro et al.	2017	118.108	-26.437	–	-3.66	2.84	–
Joshi et al.	2016	118.077	-26.428	–	–	–	–
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
Ahumada & Lapasset	2007	118.1	-26.433	–	–	–	–
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	–	–	–	–
Lynga	1987	118.121	-26.392	–	–	–	–
Sulentic et al.	1973	118.11	-26.399	–	–	–	–

💡 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–	1.35	1.07	1.19	32	0.430	631	–	0
Hunt & Reffert	2024	4.56	0.73	1.19	248	–	102⁽¹⁾	–	–
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⁽¹⁾	–	–	–	–	–	–	–
Loktin & Popova	2017	1.35	1.07	–	13	–	–	–	–
Joshi et al.	2016	1.31	1.07	–	126	–	631	–	–
Gozha et al.	2012	1.35	–	–	13	–	631	–	–
Piskunov et al.	2008	1.35	1.07	–	112	–	–	–	–
Ahumada & Lapasset	2007	–	1.07	–	13	–	–	–	0
van den Bergh	2006	1.35	1.07	–	13	–	–	–	–
Kharchenko et al.	2005	1.35	1.07	–	112	–	–	–	–
Kharchenko et al.	2003	1.35	1.07	–	–	–	–	–	–
Chen et al.	2003	1.35	–	–	10	–	–	–	–
Dias et al.	2002	1.35	1.07	–	13	–	–	–	–
Dambis	1999	1.26	0.94	–	50	–	–	–	–
Lynga	1987	3.40	1.20	–	1	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter 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	0.02

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

Visualization

ℹ️

1 2