CWNU 1610

0.11 UTI

0.25

C_N

0.57

C_dens

0.5

C_C3

0.0

C_lit

0.4

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 2.8 [N/pc²]

C3 classification BB

C_N 0.25 Poorly populated
C_dens 0.57 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1610 is a poorly populated, moderately dense object of intermediate 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant 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 1610 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–	212.948	-61.859	0.314	-7.585	-2.666	-23.811
He et al.	2023	212.949	-61.845	0.354	-7.582	-2.666	-25.21

💡 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]	B_frac	BSS
UCC	99999–	2.57	4.85	–	251	–	–	–	–
He et al.	2023	2.57	4.85	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VVV 038	60.0	213.02	-61.82	0.31	-7.59	-2.67	178.67	0.24

💡 Note: The % column shows the percentage of members that CWNU 1610 shares with each listed object.

Visualization

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