CWWDL 9741

0.02 UTI

0.55

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

N₅₀ (P>50% members) 59

Stellar density (N₅₀/rad) 22.2 [N/pc²]

C3 classification AA

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 9741 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ 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.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 9741 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–	276.738	-10.976	0.731	-1.435	-4.944	3.116
Chi et al.	2023	276.744	-10.979	0.743	-1.463	-4.945	14.367

💡 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–	–	–	–	151	-0.100	–	–	–
Chi et al.	2023	–	–	–	151	-0.100	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 347	96.6	276.74	-10.98	0.73	-1.42	-4.94	3.12	0.77

💡 Note: The % column shows the percentage of members that CWWDL 9741 shares with each listed object.

Visualization

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