CWWDL 14133

0.02 UTI

0.56

C_N

0.81

C_dens

0.75

C_C3

0.0

C_lit

0.05

C_dup

C3 classification AB

Number of members (P>50%) 61

Radius (P>50% members) 8.6 [arcmin]

C_N 0.56 Moderately populated
C_dens 0.81 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

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

Overview

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CWWDL 14133 is a moderately populated, dense object of high 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.

⚠️ 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 14133 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	–	7.377	60.51	0.646	-0.946	-0.532	-31.145
Chi et al.	2023	7.381	60.476	0.657	-0.934	-0.56	-39.607

💡 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	–	–	–	22	0.300	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 33	95.1	7.4	60.51	0.65	-0.95	-0.51	-31.8	0.6

💡 Note: The % column shows the percentage of members that CWWDL 14133 shares with each listed object.

Visualization

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