CWWDL 14596

0.10 UTI

0.3

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.27

C_dup

C3 classification CA

Number of members (P>50%) 30

Radius (P>50% members) 12.2 [arcmin]

C_N 0.3 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.27 Possibly duplicate

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

Overview

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CWWDL 14596 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near 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 14596 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	–	118.173	-42.469	3.029	-11.388	4.487	12.808
Chi et al.	2023	118.041	-42.359	3.01	-11.264	4.474	9.918

💡 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	–	–	–	3	0.270	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0450	73.3	118.08	-42.46	3.02	-11.3	4.53	14.34	0.5

💡 Note: The % column shows the percentage of members that CWWDL 14596 shares with each listed object.

Visualization

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