CWWDL 13371

0.12 UTI

0.5

C_N

0.18

C_dens

0.75

C_C3

0.0

C_lit

0.43

C_dup

C3 classification AB

Number of members (P>50%) 51

Radius (P>50% members) 10.6 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.18 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.43 Possibly duplicate

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

Overview

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CWWDL 13371 is a moderately populated, 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.

⚠️ Warning: This is possibly a duplicate object, which shares a significant 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 13371 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	–	42.855	56.886	0.41	0.318	-1.261	–
Chi et al.	2023	42.886	56.809	0.444	0.265	-1.234	-1.458

💡 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	–	–	–	0	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1244	56.9	42.99	56.84	0.39	0.37	-1.27	–	0.31
CWNU 473	25.5	42.93	56.82	0.39	0.37	-1.27	-64.95	0.01
OC 0256	17.6	42.98	56.76	0.4	0.4	-1.29	-64.95	0.03

💡 Note: The % column shows the percentage of members that CWWDL 13371 shares with each listed object.

Visualization

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