NGC 2327

(LkHalpha221)

0.00 UTI

0.66

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

N₅₀ (P>50% members) 83

Stellar density (N₅₀/rad) 73.2 [N/pc²]

C3 classification AC

C_N 0.66 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 2327 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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, and a large percentage with at least one entry reported in the same catalogue. See table with shared members information.

No fundamental parameters

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

Data

🔍 Search references for NGC 2327 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–	106.034	-11.388	0.874	-4.551	1.661	30.357
Bica et al.	2003	106.031	-11.314	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VDB 92	100.0	106.05	-11.48	0.86	-4.41	1.56	24.52	0.95
BRC27	77.1	106.03	-11.41	0.87	-4.52	1.67	30.36	0.0

💡 Note: The % column shows the percentage of members that NGC 2327 shares with each listed object.

Visualization

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