CWNU 3474

0.29 UTI

0.6

C_N

0.94

C_dens

0.75

C_C3

0.0

C_lit

0.64

C_dup

C3 classification AB

Number of members (P>50%) 69

Radius (P>50% members) 6.4 [arcmin]

C_N 0.6 Moderately populated
C_dens 0.94 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3474 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 3474 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	–	269.208	-24.302	0.487	1.146	-0.102	-18.943
He et al.	2023	269.219	-24.3	0.471	1.132	-0.101	-18.92

💡 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]	Bfr	BSS
He et al.	2023	1.82	4.65	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 73	36.2	269.26	-24.31	0.49	1.13	-0.12	-18.94	0.25

💡 Note: The % column shows the percentage of members that CWNU 3474 shares with each listed object.

Visualization

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