CWWDL 14033

0.07 UTI

0.36

C_N

0.85

C_dens

0.62

C_C3

0.0

C_lit

0.19

C_dup

C3 classification AC

Number of members (P>50%) 36

Radius (P>50% members) 5.4 [arcmin]

C_N 0.36 Poorly populated
C_dens 0.85 Dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

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

Overview

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CWWDL 14033 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 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 Very young

Data

🔍 Search references for CWWDL 14033 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	–	94.923	22.112	0.541	0.653	-2.556	25.812
Chi et al.	2023	94.921	22.078	0.538	0.629	-2.562	50.408

💡 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	-0.280	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0315	80.6	94.92	22.12	0.54	0.63	-2.53	25.81	0.51

💡 Note: The % column shows the percentage of members that CWWDL 14033 shares with each listed object.

Visualization

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