CWNU 527

0.09 UTI

0.51

C_N

0.9

C_dens

0.62

C_C3

0.0

C_lit

0.21

C_dup

C3 classification AC

Number of members (P>50%) 52

Radius (P>50% members) 4.9 [arcmin]

C_N 0.51 Moderately populated
C_dens 0.9 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.21 Likely duplicate

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

Overview

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CWNU 527 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, very young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Low extinction Metal-poor Very young

Data

🔍 Search references for CWNU 527 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	–	101.076	-3.571	0.42	-1.685	0.356	65.145
He et al.	2022	101.078	-3.561	0.43	-1.7	0.35	–

💡 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.	2022	2.69	0.06	–	3	-0.930	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1346	78.8	101.06	-3.56	0.42	-1.68	0.35	65.15	0.49

💡 Note: The % column shows the percentage of members that CWNU 527 shares with each listed object.

Visualization

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