NGC 7295

0.00 UTI

0.49

C_N

0.86

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

N_m (P>50%) 49

Core radius and density 1.4 [pc], 4.3 [pc^-2]

C3 classification AA

C_N 0.49 Poorly populated
C_dens 0.86 Dense
C_C3 1.0 Very high 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 7295 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, below 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 24 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

Data

🔍 Search references for NGC 7295 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–	336.988	52.314	0.39	-2.927	-2.761	-30.339
Dias et al.	2002	337.008	52.288	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 7296	100.0	336.99	52.32	0.38	-2.94	-2.75	-30.34	0.86

💡 Note: The % column shows the percentage of members that NGC 7295 shares with each listed object.

Visualization

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