CWWDL 1374

0.08 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 14

Core radius and density 6.8 [pc], 0.05 [pc^-2]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWWDL 1374 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 1374 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–	159.823	-59.753	0.194	-5.669	2.582	–
Chi et al.	2023	159.922	-59.788	0.208	-5.69	2.592	–

💡 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–	–	–	–	20	-0.280	–	–	–
Chi et al.	2023	–	–	–	20	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Pickard 246	12.0	159.38	-59.75	0.16	-5.68	2.59	95.94	0.05

💡 Note: The % column shows the percentage of members that CWWDL 1374 shares with each listed object.

Visualization

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