CWWDL 3744

0.12 UTI

0.0

C_N

0.1

C_dens

0.75

C_C3

0.0

C_lit

0.68

C_dup

C3 classification AB

Number of members (P>50%) 20

Radius (P>50% members) 8.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.68 Likely unique

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

Overview

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CWWDL 3744 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young 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.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 3744 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	–	33.129	57.563	0.381	-0.799	-1.067	13.372
Chi et al.	2023	33.235	57.542	0.39	-0.787	-1.078	–

💡 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
Chi et al.	2023	–	–	–	1	0.020	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 86	32.0	33.05	57.64	0.37	-0.83	-1.0	–	0.52
UBC 46	12.0	33.69	57.31	0.4	-0.83	-1.16	13.37	0.26

💡 Note: The % column shows the percentage of members that CWWDL 3744 shares with each listed object.

Visualization

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