CWWDL 13372

0.21 UTI

0.4

C_N

0.07

C_dens

0.62

C_C3

0.0

C_lit

0.95

C_dup

C3 classification AC

Number of members (P>50%) 40

Radius (P>50% members) 15.8 [arcmin]

C_N 0.4 Poorly populated
C_dens 0.07 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.95 Unique

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

Overview

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CWWDL 13372 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a metal-poor, 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 small 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=0.95) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Metal-poor Young

Data

🔍 Search references for CWWDL 13372 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	–	36.604	58.175	0.418	-0.397	-0.864	–
Chi et al.	2023	36.596	58.213	0.445	-0.356	-0.847	–

💡 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	–	–	–	44	-0.580	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13377	22.5	37.2	58.43	0.44	-0.34	-0.88	-74.78	0.06
CWWDL 13370	7.5	36.67	58.26	0.41	-0.54	-0.93	–	0.09
FSR 0596	5.0	37.48	58.13	0.4	-0.48	-0.91	-51.17	0.63

💡 Note: The % column shows the percentage of members that CWWDL 13372 shares with each listed object.

Visualization

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