NGC 2467-East

0.01 UTI

0.72

C_N

0.61

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

N_m (P>50%) 93

Core radius and density 1.6 [pc], 3.0 [pc^-2]

C3 classification AA

C_N 0.72 Moderately populated
C_dens 0.61 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 2467-East is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

No fundamental parameters

Bica et al. (2019)
2MASS website.

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for NGC 2467-East 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–	118.18	-26.382	0.201	-2.532	2.688	–
Bica et al.	2003	118.209	-26.369	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Haffner 18	96.8	118.18	-26.38	0.2	-2.53	2.63	103.52	0.73
Haffner 19	43.0	118.19	-26.28	0.2	-2.53	2.52	111.14	0.84

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

Visualization

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