CWWDL 4607

0.17 UTI

0.0

C_N

0.11

C_dens

0.75

C_C3

0.0

C_lit

0.96

C_dup

C3 classification AB

Number of members (P>50%) 23

Radius (P>50% members) 9.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

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

Overview

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CWWDL 4607 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 a unique object, which shares a very small percentage of members with at least one previously reported entry, and a significant percentage with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 4607 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	–	33.957	57.708	0.414	-0.822	-1.042	317.007
Chi et al.	2023	33.986	57.725	0.41	-0.832	-1.067	–

💡 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	–	–	–	3	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13364	56.0	34.05	57.8	0.43	-0.84	-1.05	317.01	0.14
UBC 46	4.0	33.69	57.31	0.4	-0.83	-1.16	13.37	0.26

💡 Note: The % column shows the percentage of members that CWWDL 4607 shares with each listed object.

Visualization

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