CWWDL 13480

0.09 UTI

0.0

C_N

0.22

C_dens

0.38

C_C3

0.0

C_lit

0.72

C_dup

C3 classification CB

Number of members (P>50%) 16

Radius (P>50% members) 6.8 [arcmin]

C_N 0.0 Sparse
C_dens 0.22 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.72 Likely unique

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

Overview

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CWWDL 13480 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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 likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Young

Data

🔍 Search references for CWWDL 13480 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	–	277.278	-14.261	0.521	0.13	-0.927	–
Chi et al.	2023	277.253	-14.248	0.534	0.141	-0.897	–

💡 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	–	–	–	62	-0.400	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 296	28.0	277.24	-14.25	0.52	-0.07	-0.99	22.31	0.56

💡 Note: The % column shows the percentage of members that CWWDL 13480 shares with each listed object.

Visualization

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