CWWDL 13389

0.11 UTI

0.0

C_N

0.11

C_dens

0.62

C_C3

0.0

C_lit

0.72

C_dup

C3 classification AC

Number of members (P>50%) 16

Radius (P>50% members) 8.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.62 Intermediate 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 13389 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, very 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, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 13389 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	–	131.067	-45.856	0.459	-5.09	5.059	–
Chi et al.	2023	131.202	-45.678	0.47	-5.048	5.119	31.791

💡 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	–	–	–	1	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 482	28.0	131.05	-45.93	0.46	-5.14	5.03	–	0.37
CWWDL 13552	20.0	131.51	-45.9	0.47	-5.0	5.05	–	0.08

💡 Note: The % column shows the percentage of members that CWWDL 13389 shares with each listed object.

Visualization

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