NGC 2174

(IRAS06058+2030)

0.07 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.24

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 6.0 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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NGC 2174 is a sparse, very dense object of low 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a very small 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 2174 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–	92.445	20.522	0.538	0.14	-2.367	–
Bica et al.	2003	92.461	20.503	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IRAS 06068+2030	84.0	92.45	20.51	0.52	0.17	-2.35	–	0.04
NGC 2175	76.0	92.4	20.6	0.5	0.29	-2.26	23.04	0.74
Pismis 27	8.0	92.73	20.62	0.51	-0.19	-2.05	32.5	0.78
Sh2-252C	8.0	92.33	20.65	0.48	0.19	-2.26	29.2	0.14

💡 Note: The % column shows the percentage of members that NGC 2174 shares with each listed object.

Visualization

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