CWWDL 13370

0.09 UTI

0.0

C_N

0.08

C_dens

0.5

C_C3

0.0

C_lit

0.8

C_dup

C3 classification BB

Number of members (P>50%) 19

Radius (P>50% members) 9.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.8 Very likely unique

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

Overview

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CWWDL 13370 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate 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 is very likely a unique object, which shares a 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=0.8) 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 13370 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	–	36.669	58.26	0.414	-0.543	-0.925	–
Chi et al.	2023	36.816	58.243	0.455	-0.55	-0.932	-42.819

💡 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	–	–	–	54	0.070	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 0596	20.0	37.48	58.13	0.4	-0.48	-0.91	-51.17	0.63
CWWDL 13372	12.0	36.6	58.18	0.42	-0.4	-0.86	–	0.21
CWWDL 13376	8.0	36.09	58.18	0.42	-0.65	-0.89	-67.77	0.06

💡 Note: The % column shows the percentage of members that CWWDL 13370 shares with each listed object.

Visualization

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