CWWDL 14077

0.00 UTI

0.29

C_N

0.78

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AB

Number of members (P>50%) 29

Radius (P>50% members) 5.5 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.78 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWWDL 14077 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large 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 14077 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	–	205.303	-56.674	0.585	-4.463	-1.276	-15.541
Chi et al.	2023	205.282	-56.636	0.586	-4.508	-1.282	-17.282

💡 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	–	–	–	47	-0.040	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 420	100.0	205.32	-56.67	0.58	-4.46	-1.28	-15.54	0.08
OC 0602	93.1	205.32	-56.67	0.58	-4.46	-1.28	-15.57	0.5

💡 Note: The % column shows the percentage of members that CWWDL 14077 shares with each listed object.

Visualization

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